Search for new bright nearby M dwarfs with Virtual

Máster Universitario en Astrofı́sica
Universidad Complutense de Madrid
Trabajo de Fin de Máster
Search for new bright nearby M dwarfs
with Virtual Observatory tools
Alumno:
Rubén Fedriani López
Enrique Solano
II
David Montes
Directores:
(CAB), José Antonio Caballero
IV
Tutores:
(UCM), Rosario Lorente
Septiembre 2015
I [email protected]
II [email protected]
III [email protected]
IV [email protected]
V [email protected]
I
V
III
(CAB)
(ESAC)
Resumen:
Contexto: Existen numerosas estrellas enanas M en el vecindario solar sin identificar. Estos objetos son muy importantes para los siguientes surveys de velocidad radial en la búsqueda de exoplanetas de baja masa en el infrarrojo
cercano. La identificación de estos exoplanetas es más sencilla en enanas M, en comparación con otras estrellas, tales
como G o K, debido a su favorable contraste en el cociente de radios planeta/estrella.
Objetivos: En este Trabajo Fin de Máster, buscamos estas nuevas estrellas enanas M. Preparamos una lista a partir
de una muestra suficientemente testeada de candidatos a estrellas M. Además, estimamos temperaturas efectivas,
gravedades superficiales, distancias y tipos espectrales.
Métodos: Cruzando los catálogos de CMC15 y 2MASS elaboramos una tabla de objetos. Aplicamos numerosos filtros
de movimiento propio, colores y magnitudes con herramientas de Observatorio Virtual con el objetivo de catalogar
nuevas estrellas enanas M. Inspeccionamos visualmente cada estrella usando el programa Aladin sky atlas y estimamos
parámetros astrofı́sicos con VOSA. Usamos los lenguajes de programación Python y R para estimar distancias y tipos
espectrales usando datos fotométricos de trabajos previos. Por otro lado, tuvimos la oportunidad de ir al Centro
Astronómico Hispano Alemán, gracias al Máster en Astrofı́sica con la asignatura de Técnicas Experimentales en
Astrofı́sica. Allı́, observamos espectroscopicamente con CAFOS en el telescopio de 2.2m seis de nuestros objetos.
Resultados: Hemos elaborado un catálogo de 1929 estrellas, de las cuales 849 son completamente nuevas y están
presentes por primera vez en este trabajo, y hemos estimado sus temperaturas efectivas, gravedades superficiales,
distancias y tipos espectrales. Casi 100 de nuestras estrellas pueden estar a menos de 25 pc, y otras cinco tienen
tipos espectrales M6.0 V o más tardı́o. Además, derivamos tipos espectrales de las seis estrellas observadas con
CAFOS, que están entre M4.5−5.0 V, identificando bandas moleculares tı́picas y caracterı́sticas espectrales de enanas
M. Los resultados obtenidos en la identificación visual se corresponden con los resultados estimados en nuestro estudio
fotométrico, validando nuestro trabajo.
Conclusiones: Este nuevo catálogo de 849 candidatas a estrellas enanas M ayudará a estudios relacionados con
la búsqueda de exoplanetas, estudios de estrellas frı́as en el vecindario solar y para surveys espectroscópicos en la
identificación de estrellas cercanas.
Palabras clave: Herramientas de Observatorio Virtual — estrellas: actividad — estrellas: tipo tardı́o — estrellas:
baja masa — estrellas: enanas — estrellas: parámetros fundamentales — Galaxia: vecindad — técnicas: espectrocopı́a
Abstract:
Context: There are several unidentified M-dwarf stars in the Solar neighbourhood. These objects are very important
for next radial-velocity surveys of low-mass exoplanets in the near infrared. Their identification is easier than other
kind of stars, such us G or K, because of their favourable planet/star contrast ratio radius.
Aims: In this MSc thesis, we search for such new M-dwarf stars. We prepare a list from a well tested sample of
M-dwarf candidates. In addition, we estimate effective temperatures, surface gravities, distances and spectral types.
Methods: By cross-matching CMC15 and 2MASS catalogues, we prepared a list of M-dwarf candidates. We applied
several proper-motion, colours and magnitude filters with Virtual Observatory tools in order to catalogue new Mdwarf stars. We visually inspected each target using the Aladin sky atlas and estimated astrophysical parameters with
VOSA. We developed both Python and R scripts to estimate distances and spectral types using photometric data. On
the other hand, we had the chance to go to the Centro Astronómico Hispano Alemán, within the Astrophysics Master
degree framework of the subject Técnicas Experimentales en Astrofı́sica. There, we observed spectroscopically with
CAFOS at the 2.2 m telescope five of our previously unknown objects plus a known object.
Results: We computed a catalogue of 1929 stars, of which 849 are presented for the first time in this MSc thesis, and
estimated their effective temperatures, surface gravities, distances and spectral types. Almost 100 of our stars could
be at least than 25 pc, and another five have spectral types M6.0 V or later. Besides, we derived M4.5−5.0 V spectral
types for the six stars observed with CAFOS, after identifying typical molecular bands and spectral features of M
dwarfs. These results go in the same direction of our photometric study.
Conclusions: This new catalogue of 849 new M-dwarf candidates serves for studies related with exoplanets hunting,
for studies of cool dwarfs in the solar neighbourhood and for spectroscopic surveys aiming at the identification of
nearby mid-late type M dwarfs.
Keywords: Virtual Observatory tools — stars: activity — stars: late-type — stars: low-mass — stars: dwarfs —
stars: fundamental parameters — Galaxy: neighbourhood — techniques: spectroscopy
Index
1 Introduction
1.1 A brief introduction to M dwarfs . . . . .
1.2 Search for M dwarfs using astrometric and
1.3 Why M dwarfs? . . . . . . . . . . . . . . .
1.4 Objectives . . . . . . . . . . . . . . . . . .
. . . . . . . . . . . . . .
photometric catalogues
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2 Analysis
2.1 Visual inspection . . . . . . . . . . . . . . . . . . . . . . . . . . . .
2.2 Diagrams . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
2.2.1 Colour-colour diagrams . . . . . . . . . . . . . . . . . . . .
2.2.2 Colour-magnitude diagram . . . . . . . . . . . . . . . . . .
2.2.3 Colour-reduced proper motion diagram . . . . . . . . . . .
2.2.4 Coordinates . . . . . . . . . . . . . . . . . . . . . . . . . . .
2.2.5 Histograms . . . . . . . . . . . . . . . . . . . . . . . . . . .
2.3 Spectral type estimation through photometric data . . . . . . . . .
2.4 Distance estimation through spectral type and MJ relationship . .
2.5 Effective temperature and surface gravity estimation using VOSA .
3 Results and discussion
3.1 Spectral types and distances .
3.2 Teff and log g . . . . . . . . .
3.3 Top 20 stars . . . . . . . . . .
3.3.1 Reddest . . . . . . . .
3.3.2 Fastest . . . . . . . . .
3.3.3 Nearest . . . . . . . .
3.3.4 Brightest . . . . . . .
3.4 Completeness and limiting for
3.5 Spectroscopy . . . . . . . . .
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4 Conclusions and future research
25
Appendix A: Tables
28
Appendix B: Application for Observing Time
69
1
Introduction
1.1
A brief introduction to M dwarfs
M dwarfs are the most common stars in the Solar neighbourhood, around 66%. Besides, the nearest star to the
Sun, Proxima Centauri, is a red dwarf (M5.5 V). Red dwarfs are by far the most common type of star in the Milky
Way, but they are not visible to the naked eye because of their low luminosity. The Research Consortium on Nearby
Stars( RECONS1 ) studies the nature of the Sun’s nearest stellar neighbours and according with its, the most common
spectral type in the solar neighbourhood is M. The RECONS 25 Parsec Database (Henry et al. 2006) together with
the RECONS Movie2 (Adric Riedel and the RECONS Team) allow us to know the statistic concerning the spectral
types in the Sun’s 25 pc neighbourhood, which is:
Table 1: Statistics of the Spectral Type of Sun’s 25 pc neighbourhood.
SpT
O
B
A
F
G
K
M
Number
0
1
29
141
244
550
1093
Spectral classification is based on morphology where we notice regularities in the appearance and disappearance of
particular spectral features. The traditional method of defining a spectral classification system is to take observations
of a set of stars, ideally with known absolute magnitude and luminosity class (Reid & Hawley 2005). Identifying
spectral features, strong enough to recognise in an easy way, provide us a correct classification. Particularly, M dwarfs
are main-sequence stars whose spectra display bands of TiO (Lépine & Gaidos 2011), so the TiO bands which dominate
spectra of M stars are a really good feature to be studied as a primary indicator of spectral type.
The first Morgan & Keenan (MK) system was limited in M dwarfs classification because initially it was defined
for stars with earlier type than M2 due to most photographic observations around 1940s were dominated to the blue
region where the spectral features were saturated with low temperatures (intermediate and late type M). With the
advent of larger telescopes and modern spectrographs and detectors, it became necessary to extend the classification
to later types than M2, i.e., cooler stars. There were problems between different systems, such us Yerkes and Mount
Wilson, because to the same stars they were classified as a different type. One of the problem in classifying M dwarfs
using spectra located in the blue part of the electromagnetic spectrum is that those wavelengths lie far from the peak
of the energy distribution. For this reason Boeshaar (1976) and Kirkpatrick et al. (1991), among others, extended
the MK system by adding spectral features to redder wavelengths, designated KHM system which looked for features
in the range 6300-9000 Å. There were several different systems to classify the luminosity class based on TiO or VO
bands but the more widely used is the KHM system. Nowadays the best classification is given in Alonso-Floriano et
al. (2015) and in a near future will be adopted a standardization for M.
Figure 1 shows optical spectra of late-type K and M dwarfs covering the range 3800-9500 Å. In addition, it shows
the principal spectral features. TiO is present, but weak, at K7, and grows in strength until type M6, where more
bandheads saturate. Bands due to several metal hydrides, such us MgH, FeH and CaH, also become detectable among
K7 stars and grow in prominence with later spectral type. Moreover, VO becomes evident at 7330-7530 Å and FeH
bandheads also appear in the latest spectral types at 7786, 8692 and 9020 Å. It is also remarkable the strongest atomic
lines, such us, Ca I at 4227 Å, the Na I doublets at 5890/5896 Å and 8183/8195 Å, the K I doublet at 7665/7699 Å
and finally the Ca II triplet at 8498, 8542 and 8662 Å (Reid & Hawley 2005). Considering M dwarfs as main sequence
stars with a clear spectral feature in TiO bands absorption, we can make the following summary:
• Their spectra are characterized by molecular absorption bands, mostly of TiO and VO. Besides, there are metal
hydrides, such us MgH, FeH and CaH at optical wavelengths, together with H2 O and CO in the red part of the
electromagnetic spectrum.
• They have absolute visual magnitudes between MV = 7.5 and MV = 20 mag.
• Their luminosities range from 0.2 L to less than 5 × 10−4 L .
1 http://www.recons.org/
2 https://www.youtube.com/watch?v=up_MqNBv0FE#t=171
1
• Their masses lie between 0.6 M and 0.1 M approximately and their radius lie between 0.6 R and 0.1 R
approximately. In fact, there is a roughly linear relationship between radius and masses, with a 0.4 M (0.1
M ) M dwarf having a radius of 0.4 R (0.15 R ) (Lépine & Gaidos 2011).
• Their effective temperatures lie between ∼ 3800 K (M0) and ∼ 2300 K (M9).
• They often have active chromosphere and coronae.
There are several reference providing different bounds for the previous physic parameters. Anyway all of them are
close to each other.
Figure 1: Left panel: blue optical spectra of a late K dwarfs and M dwarfs, highlighting the main features. Right
panel: red optical spectra of a late K dwarfs and M dwarfs. Molecular bands and atomic features have been highlighted
(from Reid & Hawley 2005).
In short, M dwarfs are cool, low-mass and low-radius stars. They are fully convective later than M4.0 V and mostly
convective for spectral types earlier than M4.0 V. Since the peak of the energy distribution is around 0.7-1.4 µm, it is
easier study this kind of targets in red range of the electromagnetic spectrum than in the blue-visible one (this is one
reason why we have chosen red magnitude to make our study, as explained in depth later). Whether we look for M
dwarfs on the Hertzsprung-Russell diagram, they lie on the bottom-right or lowest part of the diagram (whether we
put the diagram in the standard way, see Figure 5). Owing to M dwarfs burning their fuel very slowly, no M dwarfs
of advanced evolutionary stages exist, because of the relative short age of the Universe. Table 2, from Reid & Hawley
(2005), we summarize the fundamental properties of M dwarfs (note that we have used more recent references for our
study, but this reference is a fundamental one):
2
Table 2: Fundamental properties of M dwarfs.
Spectral type
Temperaturea
[K]
Radiusb
[R/R ]
Massc
[M/M ]
Luminosityd
[10−2 L/L ]
Log gravitye
[g cm−2 s−1 ]
M0
M1
M2
M3
M4
M5
M6
M7
M8
M9
3800
3600
3400
3250
3100
2800
2600
2500
2400
2300
0.62
0.49
0.44
0.39
0.36
0.20
0.15
0.12
0.11
0.08
0.60
0.49
0.44
0.36
0.20
0.14
0.10
∼0.09
∼0.08
∼0.075
7.2
3.5
2.3
1.5
0.55
0.22
0.09
0.05
0.03
0.015
4.65
4.75
4.8
4.8
4.9
5.0
5.1
5.2
5.2
5.4
a Temperatures
compiled from several photometric and spectroscopic calibrations.
calculated from L = 4πR2 σT 4 .
c Mass estimates from 8-parsec sample for each spectral type.
26 W.
d L calculated from M
bol using Mbol = 4.62 mag, L = 3.9 × 10
e log g calculated from g = GM/R2 .
b Radius
1.2
Search for M dwarfs using astrometric and photometric catalogues
Since the final of 20th century and the beginning of the 21th century, the way to understand photometric a astrometric
surveys has changed. With the advent of new telescopes and CCD cameras with their high and fast development,
large-scale photometric surveys have could done. Two Micron All Sky Survey (2MASS), Sloan Digital Sky Survey
(SDSS) or Carlsberg Meridian Catalogue (CMC), among others, provide us accurate, homogeneous data for huge
fractions of sky. Data from these catalogues provide us the necessary information to identify candidate stars, in our
case M dwarfs, by colour index. The point is that 2MASS is not well suited to identify nearby M dwarfs, whether it is
working alone, because J − K colour provides highly uncertain distances estimates for spectral types K5 to M7 (Reid
& Hawley 2005). But whether we combine optical/infrared colours from 2MASS and SDSS such us R − J would prove
extremely effective in selecting nearby M dwarfs. However in the past fully cross-referenced optical/infrared data sets
were not available. Nowadays, we can cross-match several catalogues using Virtual Observatory tools.
The easy access to catalogues has provided us do deeper and more complete studies. In our particular case, we
have used the last series of the Carlsberg Meridian Catalogue, CMC15 (Muiños & Evans 2014) together with the Two
Micron All Sky Catalogue- Point Sources Catalogue, 2MASS-PSC (Skrutskie et al. 2006). As we said optical/infrared
colours can provide us very good indicator studying M dwarfs, that is why we were studying the r0 − J colour (among
others). CMC15 is an astrometric and photometric catalogue in the red magnitude range from 9 to 17 magnitude,
r0 magnitude from CMC15 has a band between 0.6 and 0.75 µm. This catalogue is based on the observations of
the Carlsberg Meridian Telescope (CMT, a Grubb refractor telescope) with an objective of 178 mm diameter and
focal length 2.66 m, which is located in Roque de los Muchachos in La Palma, using a CCD camera (Kodak 2k x 2k
with 9 µm pixels) with a Sloan r0 filter operating in a drift scan mode. The observations were made between 1999
and 2011 with the CMT where the sky coverage is −40◦ < δ < +50◦ , see Figure 2. 2MASS is another astrometric
and photometric catalogue covering 99.998% of the celestial sphere in the J(1.25 µm), H(1.65 µm) and Ks (2.16 µm)
near-infrared photometric bands, see Figure 3. Observations were carried out from two dedicated 1.3 m telescopes
located at Mount Hopkins, Arizona (North Hemisphere), and Cerro Tololo, Chile (South Hemisphere). Each 2MASS
camera contains three NICMOSS3 256 x 256 HgCdTe arrays to work in the three different bands.
Besides, the use of a proper motion catalogue is a convenient way to identify nearby M-dwarf stars (nearby stars in
general), because proper motions selected samples discriminate against distant background sources including M giants
that would otherwise significantly contaminate a sample of cool stars selected by colour alone (Lépine & Gaidos 2011).
For this we also have used in our study the PPMXL catalogue of Positions and Proper Motions on the ICRS (Roeser
et al. 2010) and because neither CMC15 nor 2MASS-PSC contain no proper motions.
3
Figure 2: Sky coverage of Carlsberg Meridian Catalogue 15 presented in equatorial coordinates. Intensity is proportional to source density.
CMC15 and 2MASS-PSC together with PPMXL catalogues have been the core of our study. In addition, we used
other catalogues, such us, the ninth Data Release of the Sloan Digital Sky Survey, SDSS/DR9 (Ahn et al. 2012), the
fourth US Naval Observatory CCD Astrograph Catalog, UCAC4 (Zacharias et al. 2013) and the All sky Wide-field
Infrared Survey Explorer Data Release, AllWISE (Cutri et al. 2013) to complement our study. With SDSS/DR9 and
AllWISE we complemented the CMC15 and 2MASS information and with UCAC4 we complemented the PPMXL
information. All of them have been part of our study searching for new bright nearby M dwarfs where were managed
by VO tools.
Figure 3: Sky coverage of Two Micron All Sky Survey presented in Galactic coordinates. The image is a colour
composite of source density in the J (blue), H (green) and Ks (red) bands.
4
1.3
Why M dwarfs?
Figure 4: An artist’s conception of GJ1214b, a watery super-Earth orbiting the red dwarf GJ1214 which spectral type
is M4.5 V.
Are we the only Planetary System in the whole Galaxy or Universe? The answer is clear, no. By nature humans
are very arrogant thinking we were in the centre of the Universe, or in the centre of the Solar System. Other classic
question would be: Are we alone in the Universe? The answer now is not so clear, in my opinion no, but there are no
evidences to sustain it. The first step to find live is to find places can hold live. As first approach, by mean every star
has at least a exoplanet orbiting it, so whether in our Galaxy there are around 1,000,000,000 stars (some estimations
say even 1 trillion stars), it would be around 1,000,000,000 exoplanets just in our galaxy. Let us hunt!
In the last years several researches worldwide are looking for exoplanets around stars. In addition, NASA’s
Kepler mission in space and different instruments, such us CARMENES, are dedicated observing potential stars with
exoplanets. For example, the main goal for CARMENES is looking for low mass exoplanets orbiting mid to late M
dwarfs (Quirrenbach et al. 2014, Alonso-Floriano et al. 2015). There is a special interest in those exoplanets orbiting
in the habitable zone (HZ), which is the region around the star where a planet can have liquid water on surface. M
dwarfs are ideal targets for these missions because of their lower luminosity respect earlier spectral types. This fact
allows us easier planets detections, due to the HZ lies closer to the star. There are two principal methods to detect
exoplanets, Doppler radial velocity and transit method. M dwarfs are prime targets for exoplanets surveys because
of their low mass and bright apparent magnitude. Kepler has identified exoplanets candidates in stars with typical
colours of M dwarfs (Dressing & Charbonneau 2013, Kopparapu 2013). M dwarfs could also be used to characterize
an exoplanet’s atmosphere because of the contrast between star and planet (Kaltenegger & Traub 2009). Moreover,
in the last years there were no all sky catalogues of well characterised M dwarfs. We had to wait to the catalogues
of bright, nearby late type K and early type M dwarfs of Lépine & Gaidos (2011), with 8889 stars, and Gaidos et al.
(2014), with 2970 stars, to have a good sample on these kind of targets. In this line we want to contribute with our
1929 mid late type M dwarfs sample, which those 849 stars are presented for the first time in this MSc thesis.
Finally, being good targets for finding exoplanets, M dwarfs have very high main sequence lifetimes, in fact they
have lifetimes longer that the age of the Universe, for this reason M dwarfs can be used as a trace of the stellar
evolution in the Milky Way and the evolution of its disk (West et al. 2011).
5
1.4
Objectives
The main scientific goal for this study is the search for new M-dwarfs in order to provide a clean table to the community.
Remember that on the Hertzsprung-Russell diagram M dwarfs lie on the bottom-right, where the coolest stars lie.
Some of these stars could be study for other groups searching exoplanets. In addition, with the work developed we
are writing a paper, which will be published in next months.
Figure 5: Hertzsprung-Russell diagram showing the relative sizes of some stars. M dwarfs lie on the bottom-right part
of the Figure. Image credit: From: http://uofgts.com/Astro/allthestars.html, from Astronomy Magazine.
After the brief presentation we star to work with M dwarfs. In section 2 we explain the whole process to obtain
our sample and how we have got different estimations. In section 3 we extract all results from our study, plotting
several graphics and writing tables with the most important targets of our sample. Finally, in section 4 we highlight
the principal results and we mark the future research on this study.
6
2
Analysis
We started our analysis by cross-matching the Carlsberg Meridian Catalogue 15 (CMC15) with 134,653,515 rows and
the Two Micron All Sky Survey Catalogue with 470,992,970 rows, using 5.0 arcsec of match radius. We made this
cross-match because we are interested in the r0 magnitude from CMC15 and J, H and Ks magnitudes from 2MASS.
The cross-matching result was a table with 134,585,218 rows (that table was zeroth filter). The first filter we applied
was J < 11.5 mag, in order to consider bright targets and quite near to the Sun with 6,661,577 rows. We extended
the study of Aberasturi et al. (2014) who imposed J < 10.5 mag. Since we only want the best quality photometry
of our targets, we applied a second filter considering only the best quality flags of observation, i.e., Qf l = ‘AAA’. In
order to keep the reddest objects, we applied a third filter, r0 − J > 3.9 mag, with 1,234,728 rows. Finally, we applied
another colour filter to ensure that we are not working with giants stars, 0.8 mag < J − Ks < 1.0 mag. After applying
all these filters, we saved a table with 5023 rows. We summarise the filters in the following table:
Table 3: Filters applied to the CMC15 and 2MASS cross-match.
Filter
0th
1st
2nd
3rd
4th
Rows
···
J < 11.5 mag
Qfl=‘AAA’
0
r − J > 3.9 mag
0.8 mag < J − Ks < 1.0 mag
134,585,218
6,661,577
6,296,310
1,234,728
5023
%
Size
100
4.77
4.67
0.91
0.003
66.1 GB
4.4 GB
4.1 GB
810.2 MB
3.3 MB
We are interested in those stars with registered proper motion, so we cross-matched the 5023 rows with PPMXL
catalogue with 3.0 arcsec of match radius and we obtained 3364 rows. PPMXL and 2MASS epochs of coordinates
are the same, and similar to those of CMC15, so we did not expect losing any high-proper motion star outside the
relatively small cross-match radius of 3.0 arcsec.
As we knew many objects of our sample were in the Galactic plane, we applied an additional density filter. Dense
fields at low Galactic latitude have a lower completeness due to faint stars often being lost to nonlinearity in the
crowed areas of photographic plates (Lépine & Gaidos 2011). We made 77 visual inspections to obtain the density
along the Galactic plane in the neighbourhood of our targets. We visualised with Aladin a region with a radius of 5.0
arcmin centred on an object of our sample and we counted the number of objects in the region (see Table 4). After the
inspection, we determined the bounds of the sample in terms of Galactic latitude (l ) and longitude (b). We rejected
all objects that fell in the areas between 320 and 60 degrees in b and −10 and +10 degrees in l, plus between 60 and
75 degrees in b and -5 and +5 degrees in l. We took all objects between 75 and 320 degrees in b (see Figure 7). The
result of this cleaning was a table with 2183 rows.
Table 4: Density of the Galactic plane in term of l and b.
l/b [deg]
−15
−10
−5
0
+5
+10
+15
0
15
30
45
60
75
90
150
180
240
345
275
523
368
384
323
299
277
194
141
237
···
1088
1014
669
696
497
397
247
227
254
510
···
2391
1579
1162
1394
1119
944
827
367
318
614
1875
3451
3306
2770
2246
1937
1059
808
518
392
735
2413
2055
1546
877
1013
1426
1316
808
···
285
355
1542
1326
666
706
317
705
483
···
···
283
349
748
540
568
349
427
283
196
···
···
129
···
438
7
We plotted the data from Table 4 to see the density effect near the Galactic Centre. Figure 6 shows the stars
number with respect to Galactic longitude and latitude, respectively. There is a high concentration of objects near the
Galactic Centre reaching ∼3500 objects in just 5.0 arcmin. Furthermore, near the Galactic plane, i.e. ±10 degrees in
l, there are also high density regions. For this reason we rejected these objects because it was difficult resolve sources
on it.
Figure 6: Left panel: stars density in terms of Galactic longitude. Right panel: stars density in terms of Galactic
latitude.
We show in Figure 7 our sample distributed in Galactic coordinates after the cleaning. The subsets that we have
mentioned are shown in different colours, and the clean sample is also shown on the right panel.
Figure 7: Left panel: different rejected subsets in terms of high density. Labels show the region considered. Right
panel: clean sample after removing objects included in high density regions. Galactic coordinates are used in both
panels. Egg-like voids are areas close to the north and south equatorial poles not covered by CMC15.
All technical details on how we applied filters with TOPCAT and STILTS and the visual inspection with Aladin
can be found in M dwarfs and Virtual Observatory. An ESAC traineeship at the Centro de Astrobiologı́a (INTA-CSIC)
(Fedriani Traineship 2015).
Since we are interested in unknown objects, we cross-matched our clean sample of 2138 stars with Simbad with
a 5.0 arcsec match radius. We obtained two different tables, one of them with objects found in Simbad and another
one with objects not found in Simbad, with 1200 and 1039 rows, respectively. Since these tables have repetitions, we
inspected with Aladin one by one all objects of these tables to ensure that our final sample had no repetitions, false
sources, fakes by stellar multiplicity, multiple PPMXL sources or bad Simbad correlations. We made a Simbad script
loading the following catalogues together with an image of DDS from ESO (Garching/Deutschland- DSS.ESO, POSS
8
II): Simbad, 2MASS-PSC, CMC15, PPMXL, ALLWISE, UCAC4 and SDSS-DR9. Besides, we cross-matched with
All-sky catalog of bright M dwarfs (Lépine & Gaidos 2011) and Trumpeting M dwarfs with CONCH-SHELL (Gaidos
et al. 2014), because these objects are not in Simbad yet and we focus on unknown objects.
After the inspection, we rejected 156 rows because 79 of them had stellar multiplicity, 77 multiple PPMXL sources
and 34 were already known objects, we obtained a final sample of 849 objects. In Table A1 from Appendix, the
reader find the unknown targets not included in Simbad, with 849 M-dwarf candidates and in Table A2 the known
targets included in Simbad and Lépine & Gaidos (2011), with 1080 known stars which several of those are catalogued
as M stars.
2.1
Visual inspection
Since we are going to provide to the community a well tested table with candidates to medium-late type M dwarfs,
we made a hard visual inspection. Stringent quality control procedures, including visual confirmation of all objects,
guarantee no false detection in our table. We analysed row by row our tables using Aladin. With this inspection we
have ensured our objects’ information has no mistakes, we have ensured that they have the correct proper motion,
the correct r0 and J magnitude and they were resolved sources. Normally the process was simple because the targets
were well resolved, however, sometimes we have had to determine how the star moves in order to discern which is
the correct proper motion. Sometimes we could not resolved sources clearly because in this region there were several
objects near our target, i.e., it is a high density region. Normally in these regions the correlation was incorrect because
it takes the brightest magnitude source instead of the correct one. Besides, since there are many objects in these high
density regions there are bad correlations with PPMXL. In the practical and technical report you can find a detailed
explanation how we made this visual inspection with Aladin.
Figure 8: Left panel: a typical well resolved region. In these regions we can study perfectly our targets. Right panel:
a typical high density region is shown. We rejected this object, called CMC15 183014.3-333553, with the flag ‘stellar
multiplicity’. It is difficult to resolved catalogues sources concerning proper motions and different magnitudes in these
high density regions.
We spent several days making the visual inspection, it was a hard process, but necessary to ensure the quality
of our table. We used all catalogues that we have mentioned in Section 1. As we said these catalogues complement
each other and as they have different date we could checked the correct identification for our targets. For instance, in
Figure 9 we can see clearly how the star move just following the points from different catalogues.
9
Figure 9: Typical good correlation between catalogues. Following different points from different catalogues you can
see the proper motion of this target (CMC15 003221.4+292746) with a proper motion of µ = 79.6 mas/a
Since catalogues used in our study have different observation date we can infer the proper motion and checked
whether our target is moving in the correct way corresponding with catalogue data.
2.2
Diagrams
After the visual inspection we drew some diagrams concerning both samples unknown objects (849) and known objects
(1080). Diagrams below contain both samples where the blue points are the unknown objects and the red points are
the known objects.
2.2.1
Colour-colour diagrams
We found in the literature several colour-colour diagrams concerning M dwarfs, we drew these diagrams for our samples
and we confirmed that our M-dwarf candidates go in the direction of these studies.
Red points represent the known objects catalogued in Simbad or Lépine & Gaidos (2011), these objects are
important too because we can compare both samples, they follow the same tendency (Aberasturi et al. 2014). r0 − J
colour index is another indicator for Teff , so reddest objects, located on the left region of the left panel, also indicate
that they are the coolest objects in our sample. We know that giant stars have different colours from M dwarfs, in
the infrared colour-colour diagram we can see clearly where dwarfs have bluer J − H colours than giants, this means
that the three blue point on the upper-right corner could be giants stars. As we expected most objects are in central
region of the plot (Lépine & Gaidos 2011), proving that most of our objects are dwarfs.
10
Figure 10: Left panel: r0 − J vs J − Ks colour-colour diagram. Blue points represent the unknown objects of our
study and they are the most interesting targets for us.. Right panel: H − Ks vs J − H colour-colour diagram for the
unknown candidate objects together with the known objects.
2.2.2
Colour-magnitude diagram
A colour-magnitude diagram is a variant of the Hertzsprung-Russell diagram. In this kind of diagram we can infer
several information about spectral types and the colour of our targets. Once again r0 − J colour index indicates
that the reddest objects are the coolest one. The unknown sample lies on the bottom of the panel due to brighter
objects have already been studied; then, the brightest objects in r0 magnitude lie on the top-right. The apparently
asymptotic line crossing the panel is due to the magnitude cut in J magnitude, remember that we made the 1st which
is J < 11.5 mag; hence r0 = (r0 − J) + J and r0 cannot be larger than (r0 − J) + 11.5 mag.
Figure 11: r0 − J vs r0 colour-magnitude diagram. Our sample (blue points) are in general fainter than the objects
already known (red points) in r0 magnitude from CMC15. The most interesting objects lie on the bottom right of the
panel due to they are the reddest objects, i. e., mid-late type M dwarfs.
2.2.3
Colour-reduced proper motion diagram
Proper motion is an effective measure of identifying stars in the neighbourhood of the Sun. Since we are searching
for new bright nearby M dwarfs, we need targets with proper motions registered (PPMXL cross-matched done). The
reduced proper motion diagram provides us a great tool to divide objects of kinematically-distinct stellar populations.
We used r0 apparent magnitude to calculate the reduced proper motion Hr , which is defined by:
11
Hr = r0 + 5 log µ + 5
(2.1)
where µ is the proper motion defined by:
µ=
p
(µα cos δ)2 + (µδ )2
(2.2)
Figure 12: r0 − J vs Hr reduced proper motion diagram. The distribution in both samples unknown and known
objects are similar, however the unknown objects have Hr values lower than known objects, because the speediest
targets have already been studied.
In addition, the reduced proper motion Hr is a good indicator to distinguish giants and dwarfs stars, normally
background sources, including M giants, have a lower proper motion registered comparatively with nearby M dwarfs.
In the unknown sample there are high proper motion objects with no previous studies.
12
2.2.4
Coordinates
It is also interesting study the stellar distribution on the sky. For that reason we plot the panels below, on the left
panel we can see the distribution of our objects throughout right ascension (α) and declination (δ) in J2000, on the
right panel same as the left panel but using Galactic coordinates. It is clear that we rejected stars near both Galactic
Centre and Galactic plane. We used TOPCAT to transform the equatorial coordinates to galactic coordinates.
Figure 13: Left panel: distribution of all objects which pass the colour filters and the visual inspection in equatorial
coordinates, right ascension (α) and declination (δ) in J2000. Right panel: same as left panel given in Galactic
longitude and latitude using the standard IAU 1958 Galactic Longitude.
In Figure 13 objects have distributed uniformly along the sky, however, our unknown objects sample lie near
the galactic plane (remember we cleaned the galactic plane neighbourhood to avoid high density regions) and stellar
cluster, such us Hyades (α = 4h 27m , δ = 15◦ 520 ). There is no problem because we made the visual inspection and we
ensured that there are resolved sources. Since our catalogue is formed from CMC15 (among others) we could observed
our sample (specially the unknown objects) mostly from north hemisphere, ensuring the whole covering from Roque
de los Muchachos in La Palma (Spain).
2.2.5
Histograms
We present four diagrams with some typical values which were studied. We see on the r0 histogram that the unknown
sample is fainter than the known sample where the mean is around r0 ∼ 15.2 mag, and its distribution is close to
a Gaussian, being its minimum at ∼ 13.3 mag; in spite of the other distribution also peaks around ∼ 15.2 mag , it
reaches brighter magnitudes, around r0 ∼ 10.0 mag. Nonetheless, the faintest magnitude are close in both distributions,
17.2 mag approximately. In the J histogram we have another situation. They are still in the same direction but,
unknown objects are clearly fainter than known objects, there are more objects with faint magnitude than brighter.
On the one hand the mean of the blue distribution is 11.1 mag with minimum of 9.0 and maximum of 11.5 mag. On
the other hand the mean of the red distribution is 10.6 mag with its minimum and maximum of 5.6 and 11.5 mag,
respectively. In the case of the µ histogram the difference between samples is clear, all high proper motion objects have
already been studied as expected, new M-dwarf candidates have slower proper motions, but they are still interesting
for us. In the last panel, r0 − J histogram, we can see really close distributions, which means we are considering new
objects in our study that have consistent properties with previous works. In Table 5 is summarised the statistic of
these variables:
13
Table 5: Statistics for unknown objects.
Variable
mean
sd
min
max
r0 [mag]
J [mag]
µ [mas/a]
r0 − J [mag]
15.252
11.086
93.0
4.166
0.483
0.372
91.1
0.278
13.062
9.023
0.6
3.901
17.203
11.498
838.0
5.874
Figure 14: Top left panel: r0 histogram showing the distribution of our sample. Top right panel: J histogram
proving that the unknown objects are fainter than the known ones. Bottom left panel: µ histogram, in general we
are considering slower objects. Bottom right panel: r0 − J histogram, displaying a similar distribution between both
samples.
In conclusion, in this section we show that we are studying the objects never studied for other groups, faint objects,
not high proper motion, sometimes in high density region, such us near to Galactic plane or stellar cluster. Nevertheless
both samples are in the same direction.
14
2.3
Spectral type estimation through photometric data
Deep wide multi-band photometric compilations of different catalogues are an useful tool for the estimation and
assignment of spectral types. Owing to M dwarfs are better understanding in the red region of the electromagnetic
spectrum, we have r0 magnitude from CMC15, J and Ks magnitudes from 2MASS which are red magnitudes, with
that we calculated the colour index r0 − J and r0 − Ks which are representative colour index for M dwarfs. There
are several previous works which found a relationship between a colour index and expected spectral types (Lépine &
Gaidos 2011, West et al. 2011, Holgado 2014, Aberasturi et al. 2014), or temperatures (Kaltenegger & Traub 2009).
We decided use photometric data to estimate spectral type because the estimation through temperature introduce high
uncertainty. With both colour index we can estimate the spectral type just using photometric data, we use estimation
from Holgado (2014), which is being used by the CARMENES3 consortium4 .
We expected intermediate-late type M dwarfs (≥ M4.0 V) because of the colour filters applied, so using data from
Table 10 of Holgado (2014) (Tabla 10: Valores medios de los ı́ndices de color ) we estimated spectral types from colour
index r0 −J where we found a quadratic relation between those, hence in order to be more accurate we made a weighted
quadratic fit with the available data.
Table 6: Colour index vs Spectral Type.
SpT
r0 − J
[mag]
M0.0 V
M0.5 V
M1.0 V
M1.5 V
M2.0 V
M2.5 V
M3.0 V
M3.5 V
M4.0 V
M4.5 V
M5.0 V
M5.5 V
2.49±0.25
2.48±0.09
2.63±0.12
2.79±0.11
2.93±0.09
3.05±0.14
3.25±0.10
3.49±0.12
3.71±0.13
4.04±0.18
4.47±0.21
4.90±0.28
r 0 − Ks
[mag]
3.32±
3.32±
3.47±
3.62±
3.77±
3.90±
4.10±
4.33±
4.56±
4.90±
5.38±
5.82±
0.26
0.11
0.13
0.12
0.10
0.13
0.11
0.12
0.16
0.20
0.24
0.27
We can see the result of this fit in Figure 15 which was made in R. This fit define the bounds to determine, given
a colour index, which spectral type correspond.
Figure 15: Weighted quadratic fit made in R. Black solid points represent points given in Table 6 and vertical lines
represent the error. Red line is the quadratic fit and red solid squares represent the colour index considered for each
spectral type defining ours boundaries.
3 Calar
Alto high-Resolution search for M dwarfs with Exoearths with Near-infrared and optical Échelle Spectrographs.
4 https://carmenes.caha.es/
15
Note that whether a star has a colour index r0 − J greater than 4.90 we derived their spectral type thanks to the fit,
we extended the definition and we can reach the spectral type M6.0 V. There is an intrinsic error of ±0.5 concerning
the spectral type, that is the minimum uncertainty in spectral type. There are 20 stars with a colour index r0 − J
greater than 4.98. These targets are very interesting because are the reddest one in our sample. We will explain in
depth in Section 3.
In Fedriani Traineship (2015) you can find a discussion about which is the best colour index estimation between
West et al. (2011) and Holgado (2014) and why we finally took the Holgado estimation. Besides, you can find the
code developed in Python and R concerning these tasks. In this way we redefine the boundaries to estimate spectral
types given r0 − J colour index, see Table 7.
Table 7: Colour index vs Spectral Type new boundaries.
2.4
r0 − J [mag]
SpT
r0 − J [mag]
SpT
[2.51, 2.54)
[2.54, 2.61)
[2.61, 2.71)
[2.71, 2.86)
[2.86, 3.03)
[3.03, 3.25)
[3.25, 3.50)
M0.0 V
M0.5 V
M1.0 V
M1.5 V
M2.0 V
M2.5 V
M3. V
[3.50, 3.78)
[3.78, 4.11)
[4.11, 4.47)
[4.47, 4.86)
[4.86, 5.29)
[5.29, ∼ 5.7)
& 5.7
M3.5 V
M4.0 V
M4.5 V
M5.0 V
M5.5 V
M6.0 V
> M6.0 V
Distance estimation through spectral type and MJ relationship
After obtaining spectral types through photometric data in the previous section, now we can obtain absolute magnitude
MJ . There are different relationships between spectral type and absolute magnitude (Hawley et al. 2002, Pecaut et
al. 2012, Pecaut & Mamajek 2013). We adopted one of the last relationships because the M standards have changed
significantly since the 1950s-1970s, and the 1990s used by Kirkpatrick, Henry, and collaborators. Older compilations
of colours in relation with other astrophysics parameters from 1980s and early 1990s are likely to be out of date, so
this fact helps us to use recent compilation with modern M standards.
We used a relationship between spectral type and absolute magnitude MJ given in “A Modern Mean Stellar Color
and Effective Temperature Sequence for O9V-Y0V” by Eric Mamajek5 (University of Rochester). Part of this table is
into Pecaut et al. (2012) and Pecaut & Mamajek (2013), but not all, we only used the relation mentioned, see Table
8.
Table 8: Spectral Type vs MJ .
SpT
M0.0 V
M1.0 V
M2.0 V
M3.0 V
M4.0 V
M5.0 V
M6.0 V
MJ [mag]
6.14
6.54
6.89
7.40
8.39
9.25
10.28
Using the relation given in Table 8 we made a quadratic fit in order to infer the MJ value of each subspectral type.
We created a R script for this task, we made the quadratic fit and then we obtained the points in our curve to define
our boundaries to assign absolute magnitudes, see Figure 16 and Table 9.
5 You
can find the whole table in: http://www.pas.rochester.edu/~emamajek/EEM_dwarf_UBVIJHK_colors_Teff.txt
16
Figure 16: Quadratic fit made in R. Black filled points represent points given in Table 8. Blue line is the quadratic fit
and blue solid squares represent the MJ value considered for each spectral type defining ours boundaries.
Table 9: Spectral Type vs MJ .
SpT
M0.0 V
M0.5 V
M1.0 V
M1.5 V
M2.0 V
M2.5 V
M3.0 V
M3.5 V
M4.0 V
M4.5 V
M5.0 V
M5.5 V
M6.0 V
MJ [mag]
6.17
6.29
6.46
6.67
6.91
7.20
7.52
7.88
8.29
8.74
9.22
9.74
10.31
So given a spectral type we can infer its MJ , that is, given a r0 − J colour index we can infer a spectral type
and hence a MJ . As before, we define new values obtained in the fit, see Table 9. Once we have estimated absolute
magnitudes MJ for each object in our sample we can obtain distances. For this, we used the well-known formula:
m − M = 5 log d − 5
(2.3)
being m = J and M = MJ . Since we are working with stars in the Solar neighbourhood (. 45 pc), we considered a
null extinction, AJ ≈ 0 mag in our distances estimations. In Section 3 we present the distances distribution which is
consistent with our study.
2.5
Effective temperature and surface gravity estimation using VOSA
Astrophysical parameters, such us temperatures and surface gravities, are fundamental to understand the properties of
a star. The Virtual Observatory tool VOSA (Virtual Observatory SED Analyzer6 ) developed by the Spanish Virtual
Observatory (SVO), which has been described in Fedriani Traineship (2015), allow us to estimate these parameters. We
have to upload a plain text with the names and coordinates of the objects, after that VOSA collects all VO photometry
available for our objects. With this photometry VOSA creates synthetic SED’s, besides using chi-squared and Bayesian
fits VOSA can estimate effective temperature and surface gravity for each object. To do that, VOSA compares for
each object its SED with those derived from theoretical spectra obtained from VO services. There are several models
available7 to make the fit, but we used the BT-Settl-CIFIST theoretical model which is integrate in the last version
of VOSA. We can choose the parameter ranges for temperatures (Teff ), surface gravities (log g) and metallicity (meta)
for both fit chi-squared and Bayesian. We made the fit with the following values: Teff ∈ [2000, 4000] K, log g ∈ [3.5, 5.5]
and meta=0, being typical values for M dwarfs (notice that we have put conservatives bounds, in order to work with
all parameters space). The difference between chi-squared and Bayesian model is that the Bayesian model also gives
a probability of this particular parameters (Teff and log g).
We expect temperatures around ∼ 3100 K, with a maximum value ∼ 3200 K and a minimum value ∼ 2500 K.
Regarding the surface gravities, we expect surface gravities around log g ∼ 5.0, with a maximum value log g ∼ 4.8 and
minimum value log g ∼ 5.2. In Section 3 we show the histograms of these parameters.
6 http://svo2.cab.inta-csic.es/theory/vosa50/index.php
7 We
collect the available models in Appendix of Fedriani Traineship (2015).
17
3
Results and discussion
We present a catalogue of 1929 stars. Of them 1080 stars are already catalogued in Simbad or Lépine & Gaidos
(2011) (see Table A2), and 849 stars are completely new (see Table A1), they are presented for the first time in this
MSc thesis. As explained in detail below, we derived spectral types and distances through photometric data and we
estimated Teff and log g using VOSA. Besides, we observed spectroscopically six stars of our catalogue confirming our
study. In the following subsections we present the results concerning only the unknown sample.
3.1
Spectral types and distances
In Figure 17 we present the spectral type histogram for our 849 M-dwarf candidates. We have obtained the expected
results, i.e., mid-late type M stars (≥ M4.0 V). According to our estimates we got 475 stars with M4.0 V spectral
type, 270 with M4.5 V, 73 with M5.0 V, 26 with M5.5 V, 4 with M6.0 V and one later than M6.0 V. We expected this
distribution of spectral types where earlier types dominated over later types, it is normal because late type M dwarfs
are fainter than earlier types and it is more difficult to find. We obtained 104 stars with a spectral type M5.0−6.0 V
which are very interesting targets.
Figure 17: Spectral type histogram.
The results obtained in the distance estimation verify our initial constrain, we wanted to study the solar neighbourhood, that is, d ∼ 30 pc. In Figure 18 we present the distances histogram where the mean of the distribution is
d¯ = 32.6 pc. The minimum value of the sample is 9.5 pc and the maximum is 43.7 pc. The results obtained have been
the expected values, being these near stars very important for other groups aiming the catalogue of the nearest stars
in the Solar neighbourhood.
Figure 18: Distances histogram.
18
3.2
Teff and log g
Using the VO tool VOSA we obtained Teff and log g through the VO photometry collected for each object. In Figure
19 we present Teff and log g histograms. On the one hand, the temperatures distribution explain mainly our unknown
sample, but there are some outlier values on the tails because we do not expect objects with high temperature
(> 3200 K) and with very low temperature (< 2500 K). Due to we have spectral types between M4.0−6.0 V we expect
temperatures between 3100−4200 K that they are the most common in our histogram, besides the mode is ∼ 3100 K
which corresponds with the mode in the spectral type M4.0 V (if we take the median, which is a robustness measure of
position avoiding outlier values, we obtain 3100 K as well, and M4.0 V), showing that mainly the histogram is correct.
On the other hand, the surface gravities distribution is a bit far from our expected values because we expected log g
between 4.9−5.1 and we obtained values between 3.5−5.5 (see right panel of Figure 19). The reason of this difference
could be the grid size of the theoretical model, because it is a step of 0.5 in log g, which very high considering that
we want a precision of 0.1. Actually it is not a problem in the tool just in the grid of the theoretical model BTSettl-CIFIST. Notice that the most common bins are 4.5 and 5.0 in log g, which correspond with our spectral type
estimation (see Table 2), hence when we have a smaller grid size in the theoretical model we could be more accurate
and obtain better results in log g.
Figure 19: Left panel: effective temperatures histogram. Right panel: surface gravities histogram.
3.3
Top 20 stars
In this section we present the most interesting objects that we found in our unknown sample attending different
properties, such us colour index, proper motion, distance and magnitude. To make these tables we have considered
objects with a proper motion greater than 30 mas/a (µ > 30 mas/a) to ensure that they are potential M-dwarf
candidates, because with a low proper motion the objects could be background or giant stars. This filter was also
applied for other authors cataloguing M dwarfs (Lépine & Gaidos 2011, Gaidos et al. 2014) considering µ > 40 mas/a,
however, they used the USNO-B1 catalogue which is less accurate than the PPMXL catalogue. With a cut in µ of
30 mas/a we are considering 6σ in velocities dispersion in PPMXL catalogue, hence we are considering equivalent
proper motion cut as previous authors. With this filter, we keep 676 stars (80% of the final unknown sample), being
the remainder also interesting objects, because we can do other type of research with it (see Section 4). From this
point each table presented has the first column with a number (No.) which is the identifier of the star to refer them
and find easily in the complete table (Table A1), where the reader can find more additional information about the
stars presented in the following tables.
19
3.3.1
Reddest
In Table 10 we present the top 20 reddest objects considering the colour index r0 − J. These objects are at the same
time, obviously, the latest type of our sample to M-dwarf candidates. Notice that object No. 46, 336, 597, 230, 357
appear in Table 12, where we tabulate the nearest objects. It makes sense because if we identify this late-type object
they should be near to us because they are very difficult to find far away due to they are much fainter.
The object No. 46 is the reddest object in our sample with a colour index of r0 − J = 5.874 mag and it is at the
same time the latest type in our sample. We think that it could be later than M6.0 V because when we made the
spectral type estimation, the colour index r0 − J was greater than the maximum value for our quadratic fit which
correspond with M6.0 V. For this reason we think that, perhaps, the star could be M6.5 V which would became a
really interesting object because there are several groups worldwide searching for such late-type M dwarfs. These
reddest objects are perfect to observed and find more information about them.
Table 10: Top 20 reddest.
No.
CMC15
r0
[mag]
J
[mag]
Ks
[mag]
SpT
r0 − J
[mag]
46
336
597
230
357
492
474
576
103
644
658
676
44
449
548
438
715
835
105
464
022957.4−360639
111548.1+274616
164049.9−261653
062920.1+172516
122150.1+463244
154910.6−352307
153348.6−291126
162632.7−262259
041950.2+292647
174919.2+475605
183801.5+341806
190543.4−271125
021922.1−392522
152012.7−355925
161703.3−214102
150950.9+150250
201822.7+000507
232416.9−152223
042044.6+180558
153013.7−140144
17.203
16.735
16.694
16.551
16.584
16.670
16.344
16.685
16.596
16.438
16.561
16.291
16.466
16.523
15.967
16.435
16.370
16.144
16.129
16.178
11.329
11.284
11.282
11.162
11.259
11.383
11.105
11.452
11.369
11.214
11.419
11.152
11.381
11.472
10.971
11.450
11.387
11.190
11.194
11.243
10.340
10.324
10.386
10.302
10.286
10.414
10.272
10.490
10.473
10.285
10.526
10.259
10.404
10.639
10.047
10.525
10.447
10.196
10.313
10.396
>M6.0 V
M6.0 V
M6.0 V
M6.0 V
M6.0 V
M5.5 V
M5.5 V
M5.5 V
M5.5 V
M5.5 V
M5.5 V
M5.5 V
M5.5 V
M5.5 V
M5.5 V
M5.5 V
M5.5 V
M5.5 V
M5.5 V
M5.5 V
5.874
5.451
5.412
5.389
5.325
5.287
5.239
5.233
5.227
5.224
5.142
5.139
5.085
5.051
4.996
4.985
4.983
4.954
4.935
4.935
20
3.3.2
Fastest
In Table 11 we tabulate the fastest objects in our sample. These objects with high proper motion have high probabilities
of being M dwarf, because there are no giant stars with these high proper motions. The fastest objects lie on the
bottom of the Hr diagram (see Figure 12), because of the definition of the reduced proper motion. Take into account
that we have to consider the proper motion with the r0 magnitude, so a higher reduced proper motion does not imply
a higher proper motion. All of these objects have a proper motion µ > 380 mas/a, and there are more than 300 objects
with a proper motion greater than 100 mas/a, being ideal targets to be considered. Notice that object No. 662, which
is the fastest one, is also one of the nearest one (see Table 11), being a good target to observe in next campaigns.
Besides, object No. 669 is one of the targets that we observed spectroscopically at CAHA (see Table 15 and Figure
21). Finally, object No. 644 is also one of the brightest stars (see Table 13), being another good target to observe.
Table 11: Top 20 fastest.
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
Hr
[mas/a]
µ
[mas/a]
662
598
426
235
669
470
198
89
20
313
368
207
465
644
308
208
205
267
295
101
184249.7−321247
164109.9−225444
144713.8−321739
063051.5−065809
185955.9+432359
153140.8+021042
053506.4−170633
035342.3−252700
011113.4+030640
101107.6−053328
124358.7−161434
055128.1−153034
153021.8−135846
174919.2+475605
100009.7+064703
055204.0+355027
054801.0−250104
075313.5−101219
090913.2−021611
041806.4−240626
−673.3
+207.6
+596.3
+350.6
+351.4
+14.6
+480.3
−326.3
−385.7
−352.2
−429.2
−233.9
−163.0
−408.7
−356.9
−19.1
−102.8
+146.3
+90.6
−115.3
−498.6
−793.2
−478.5
+406.2
+396.6
−529.2
−92.2
−348.3
−280.0
−261.8
+82.3
+352.8
−385.8
+86.5
+212.7
+414.1
+384.2
−360.5
+375.1
−368.1
18.1
19.8
20.1
18.6
18.4
19.3
17.7
18.0
18.1
18.4
17.3
18.5
18.5
19.5
18.0
18.3
18.4
18.8
18.1
18.3
837.8
819.9
764.5
536.6
529.9
529.4
489.1
477.3
476.6
438.8
437.0
423.3
418.8
417.8
415.5
414.5
397.7
389.1
385.9
385.7
21
3.3.3
Nearest
In Table 12 we tabulate the nearest objects according with our estimations. These 20 objects are in our solar
neighbourhood at a distance less than 20 pc. One of the most interesting results in our work is these nearest objects
because we can contribute with the census of the nearest stars in the solar neighbourhood. In this table we only list the
20 nearest, but there are almost 100 object with a distance d < 25 pc. According to previous research around ∼ 66%
of the stars in the Solar neighbourhood are M stars (the 100 nearest stars meet this percentage8 ). The RECONS
group (Henry et al. 2006) is carrying out the census of the nearest stars considering distances less than 25 pc (see
Table 1), taking this information we can infer the currently percentage of M, it is just 1093/2058≈0.53. Extrapolating
the information of the 100 nearest stars, how many M stars do we need to complete this percentage? With this simple
relation we obtain it:
1093 + x
= 0.66
2058 + x
where x is the M stars needed. Solving for x we can write:
(3.1)
0.66 · 2058 − 1093
≈ 780 stars
(3.2)
0.34
We found in our sample 97 M-dwarf candidates with d < 25 pc, which meet with the requirements of the RECONS
group searching the nearest stars. When our paper is accepted and our work confirmed, we can provide the ∼12%
of these nearest stars unknown. In next years Gaia will resolve this task confirming the distances and parallaxes for
several stars.
As we said in the previous subsection, objects No. 230, 357, 597, 336 and 46 are also in Table 10 being the reddest
objects as well.
x=
Table 12: Top 20 nearest.
No.
CMC15
SpT
d
[pc]
573
230
357
597
336
46
368
547
282
397
332
527
548
662
441
722
474
781
220
162416.4−321213
062920.1+172516
122150.1+463244
164049.9−261653
111548.1+274616
022957.4−360639
124358.7−161434
161658.8−313638
084040.8−383238
135821.6−004626
105850.4−234620
160905.2−080946
161703.3−214102
184249.7−321247
151355.4−394114
202527.1−194803
153348.6−291126
211757.1+460130
061114.6−003537
M4.5 V
M6.0 V
M6.0 V
M6.0 V
M6.0 V
M6.0 V
M4.5 V
M4.0 V
M4.5 V
M5.5 V
M5.0 V
M5.0 V
M5.5 V
M4.0 V
M5.0 V
M4.5 V
M5.5 V
M4.0 V
M5.0 V
12.1
14.8
15.5
15.6
15.7
16.0
16.1
16.1
16.2
16.3
16.4
16.8
17.6
17.8
17.9
18.2
18.7
18.9
19.1
8 http://www.recons.org/TOP100.posted.htm
22
3.3.4
Brightest
In Table 13 we tabulate the brightest objects, in r0 magnitude, for our sample. They are mainly early types (M4.0 V)
because the colour index r0 − J could not be so high. Notice that object No. 662 is the fastest object in our sample
and one of the brightest objects as well. These stars are the easiest one to observe. We encourage the observation of
these targets in future campaigns.
Table 13: Top 20 brightest.
3.4
No.
CMC15
r0
[mag]
J
[mag]
Ks
[mag]
573
547
662
673
781
377
51
232
282
91
368
174
845
92
198
475
284
722
646
300
162416.4−321213
161658.8−313638
184249.7−321247
190259.2−202239
211757.1+460130
131640.5−085825
024816.8+053705
063001.8−192336
084040.8−383238
035624.6−311138
124358.7−161434
051429.4+091807
234208.6+010918
040044.9+135422
053506.4−170633
153444.6−280026
084615.3+040638
202527.1−194803
180113.4+094837
092311.4−352313
13.321
13.394
13.451
13.687
13.698
13.954
14.026
14.052
14.087
14.090
14.113
14.130
14.192
14.209
14.209
14.260
14.268
14.284
14.286
14.306
9.150
9.329
9.544
9.738
9.673
10.043
10.072
10.092
9.790
10.072
9.777
10.103
10.194
10.260
10.178
10.332
10.244
10.042
10.294
10.404
8.154
8.475
8.679
8.889
8.807
9.199
9.162
9.254
8.868
9.121
8.896
9.241
9.313
9.344
9.295
9.422
9.320
9.149
9.369
9.584
Completeness and limiting for the CARMENES input catalogue
There is a star subsample in our unknown star sample very interesting for currently surveys. In Table 1 of AlonsoFloriano et al. (2015) they define a strict requirement in order to keep with the most favourable targets to observe.
They were selected according to mid-late spectral type and brightness. In Table 14 we write the table of the paper,
with the requirements of the CARMENES input catalogue, alongside with the stars in our sample that meet with these
requirements. The point to meet this requirement in J-band magnitudes per spectral type is the following: if we have
a star with a specific spectral type, for instance M4.0−4.5 V, the J magnitude has to be less or equal than the values
written in the columns of completeness and limiting, being the limiting value the maximum allowed value considered
for the CARMENES input catalogue. In our sample there are 65 stars meeting the limiting requirement, where 48
are M4.0−4.5 V, 12 M5.0−6.0 V and 5 of them M6.0−6.5 V, and one of them also meeting with the completeness
requirement. These objects could be part of the CARMENES input catalogue searching for exoplanets around M
dwarfs, but they also have to meet other coordinate requirement, i.e., stars must be observable from Calar Alto with
target declination δ > −23 deg. The object which meets the completeness requirement is CMC15 162416.4-321213
(No. 573) which is a M4.0 V star with high proper motion (µ573 = 169.5 mas/a). However, this object does not meet
with the coordinate requirement (δ573 = −32.20364 deg), hence it could not be part of the input catalogue. If we
take only the objects which pass the limiting requirement with δ > −23 deg, we keep with 40 stars (29 M4.0−4.5 V, 8
M5.0−5.5 V and 3 M6.5−6.5 V), being these 40 stars really interesting targets for the CARMENES input catalogue,
in fact the CARMENES panel are planning to include these stars in the catalogue. Nonetheless, the star which meets
completeness requirement and the 25 reminder in the case of limiting could be interesting for other surveys, such us
23
HARPS9 which is a survey from the European Southern Observatory (ESO) hunting exoplanets.
Table 14: Stars that pass the CARMENES input catalogue selection criteria.
Spectral type
M0.0-0.5 V
M1.0-1.5 V
M2.0-2.5 V
M3.0-3.5 V
M4.0-4.5 V
M5.0-5.5 V
M6.0-6.5 V
M7.0-7.5 V
M8.0-9.5 V
3.5
J [mag]
Completeness Limiting
7.3
8.5
7.8
9.0
8.3
9.5
8.8
10.0
9.3
10.5
9.8
11.0
10.3
11.5
10.8
11.5
11.3
11.5
Our sample
Completeness Limiting
0
0
0
0
0
0
0
0
0
48
1
12
0
5
0
0
0
0
Spectroscopy
On 8th and 9th April 2015, we used the Calar Alto Faint Object Spectrograph at the 2.2 m telescope, CAFOS 2.2, in
the Centro Astronómico Hispano-Alemán (CAHA), Calar Alto (Almerı́a). CAFOS is a focal reducer which provides
the facilities for do direct imaging and spectroscopy with grisms and longslit, moreover we can do polarimetry and
imaging through a Fabry-Pérot etalon, with at spectral resolution R ≈ 82000. We used the configuration with both
grisms G100 and R100. G100 has a coverage wavelength from 4900 and 7800 Å and R100 from 5900 and 9000 Å which
allow us to determine the spectral type of our targets.
We knew that we had a unique opportunity to validate our study, so we proposed to the responsible of the subject
Técnicas experimentales en Astrofı́sica, Jaime Zamorano, observing our own targets that we had been studied during
our traineeship at CAB-ESAC. We made a real application for observing time to CAHA10 .Finally, we collected low
resolution spectra of 6 M-dwarf candidates, which are shown in Table 15 where we indicate some properties of our
targets, besides we put the estimated spectral type made with our photometric study. Exposure times ranged between
350 and 2400 s, depending of the target brightness. Raw data were reduced with standard procedures within the IRAF
environment, bias and flat-field correction, cosmic-ray rejection, spectra extraction, wavelength calibration using CuNe-Ar arc lamps taken during the observation, spectra calibration. Every M-dwarf candidates are unknown objects,
less the star No. 693 which is already studied by Lépine & Gaidos (2011) (see Table A2).
Table 15: Observed stars with CAFOS.
No.
CMC15
273
693
467
643
669
691
081202.5+070932
141707.3+085136
153116.7+344126
174814.3+133747
185955.9+432359
193620.0+354736
α(J2000)
[deg]
123.010691
214.280502
232.81972
267.059614
284.982935
294.083602
δ(J2000)
[deg]
7.159164
8.860157
34.690684
13.629873
43.399788
35.793454
µα cos δ
[mas/a]
+77.5
−139.4
−101.3
−63.5
+351.4
+156.5
µδ
[mas/a]
+74.4
+17.9
+39.8
−85.3
+396.6
+89.5
Hr
[mas/a]
14.7
14.0
14.8
14.9
18.4
15.8
r0
[mag]
14.546
13.229
14.640
14.779
14.749
14.488
r0 − J
[mag]
4.009
4.120
3.908
4.445
4.022
4.061
SpT
(photometric)
m4 ±0.5
m5±0.5
m4±0.5
m4.5±0.5
m4±0.5
m4±0.5
SpT
(spectrum)
M4.5 V
M4.5 V
M5.0 V
M5.0 V
M4.5 V
M4.5 V
The result of the observation and data reduction was the following spectra of our M-dwarf candidates, see Figure
20 and 21.
9 HARPS
10 Find
- High Accuracy Radial velocity Planet Searcher http://www.eso.org/sci/facilities/lasilla/instruments/harps.html
the whole application in Appendix B.
24
Figure 20: CAFOS/CAHA spectra our M-dwarf candidates with G100 grism.
Figure 21: CAFOS/CAHA spectra of our M-dwarf candidates with R100 grism.
On spectra above we identified spectral features, such us molecular bands (TiO, CaH, H2 O band, O2 A-band, VO),
lines and doublets (Hα, Hβ, KI, NaI). We obtained spectral types through the comparison with spectra collected in
Alonso-Floriano et al. (2015). In Table 15 we wrote both spectral types through photometric estimation and visual
comparison identifying typical features, as we see there are to close, validating our work. Considering the errors, using
photometric data to estimate spectral type or doing spectroscopy are almost the same, for sure the most accurate
procedure is to take the spectra and determine their spectral type, but we can reach a really good approximation
using our study in order to manage big number of stars.
4
Conclusions and future research
Taking advantages of VO tools, we present a catalogue with 1927 stars, which 1080 are already known stars and
849 are unknown M-dwarf candidates. We cross-matched the photometric CMC15 (r0 ) and 2MASS (J) catalogues
applying several filters to constrain our sample using VO tools. We also showed the potential and importance of the
Virtual Observatory, working with VO tools and data archive, for finding new nearby bright mid-late type M dwarfs.
Perhaps, some stars catalogued by us can host exoplanets and who knows if their exoplanets can have liquid water
hosting life in them, we will know in a near future.
We estimated distances and spectral types for the unknown sample through photometric relationships, obtaining
expected results. In addition, we derived effective temperatures and surface gravities for each star using VOSA.
Our work could increase the census of the nearest objects providing 97 stars with distances less than 25 pc. In a
few months, when we have information from Gaia, we will be able to confirm our study. Our catalogue includes many
stars which are identified here for the first time as members of the solar neighbourhood. In particular, most of the
sources are not listed in the Catalog of the Nearby Stars. Besides, we contribute with 40 stars to the CARMENES
25
input catalogue in order to search exoplanets orbiting these M-dwarf stars, which are low-mass stars being easier to
detect extra-solar planets in habitable zones with relatively low masses.
We used the Calar Alto Faint Object Spectrograph at the 2.2 m telescope, CAFOS 2.2, in the Centro Astronómico
Hispano-Alemán (CAHA), Calar Alto (Almerı́a) for obtaining low-resolution optical spectroscopy of 6 targets, 5 of
them had not been spectroscopically analysed before. We did not obtain spectra of the rest of the sample, but we
encourage community involvement to complete the spectroscopy survey or Radial Velocity (RV) monitoring programs.
The next generation of extremely large ground based telescopes and space telescopes, such us the James Webb Space
Telescope, will have an important role observing such stars hosting exoplanets.
Future research: We have to validate the objects with a proper motion greater than 40 mas/a, on the other hand
objects with less than 40 mas/a are very interesting because with the colour filter applied could be interesting giants
objects in the middle of star supercluster, we have to study the spatial distribution in the Hyades cluster. Besides,
we found several objects with X-ray emission so we can correlate with the ROSAT catalogue in order to find active
stars. We also found several pairs that could be wide companion, so in a future research we will investigate in deep
these pairs. This MSc thesis have been the first step for a refereed paper.
26
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27
Appendix A: Tables
Table A1: New M-dwarf candidates (not in Simbad).
No.
CMC15
α(J2000)
[deg]
δ(J2000)
[deg]
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
000238.8−214833
000453.0−103220
000636.3−090603
001024.0−262321
001652.4+085041
001931.9−055440
002111.3−084140
003221.4+292746
003237.2+391100
003244.5+274444
004036.0+335408
004217.6−035443
004434.5+160701
004725.0+480327
004826.6−184720
005020.4+175109
005410.3+050928
005548.5−151745
010301.3+065849
011113.4+030640
011131.4−110017
012127.0+051925
012645.2−360942
013035.3+200839
013055.3−332904
013304.4−063128
013958.2+464259
014101.6+433550
014256.1+342622
014516.7+163658
014947.9−133633
015139.5+465240
015324.4−342611
015730.6+391824
015736.3−305828
015901.0+360955
020150.7−072658
020837.0+261713
021156.3−014215
021437.7+243548
021521.1−390918
021548.3+205755
021750.5+082950
021922.1−392522
022213.6−054919
022957.4−360639
0.661843
1.221038
1.651329
2.600022
4.218501
4.883245
5.297174
8.089319
8.155314
8.185711
10.150005
10.573443
11.144141
11.854270
12.111222
12.585207
13.542933
13.952250
15.755602
17.806162
17.880854
20.362627
21.688385
22.647405
22.730673
23.268607
24.992527
25.257006
25.734099
26.319958
27.449697
27.914695
28.351723
29.377507
29.401477
29.754415
30.461581
32.154523
32.984700
33.657094
33.838199
33.951614
34.460648
34.842403
35.556795
37.489289
−21.809337
−10.538929
−9.100843
−26.389441
8.844823
−5.911376
−8.694606
29.462960
39.183407
27.745740
33.902487
−3.912215
16.116962
48.057735
−18.789064
17.852661
5.158032
−15.296101
6.980333
3.111346
−11.004819
5.323838
−36.161740
20.144224
−33.484685
−6.524537
46.716471
43.597312
34.439719
16.616383
−13.609309
46.877963
−34.436439
39.306719
−30.974520
36.165433
−7.449626
26.287176
−1.704377
24.596777
−39.155151
20.965303
8.497300
−39.423039
−5.822085
−36.111097
−106.7
+62.4
−164.8
+74.3
−12.2
+111.4
−62.7
−62.7
−9.6
+87.3
+117.1
−12.0
+52.7
+39.9
+70.0
+70.2
+39.5
+46.0
−82.6
−385.7
−42.0
−7.9
+153.1
+50.4
+118.8
−53.8
−16.8
+48.1
+88.4
−74.2
+62.4
+46.8
−31.3
−59.4
−23.5
+74.0
+96.7
−102.2
+94.0
+107.1
+118.6
+31.2
+54.7
+106.0
+19.1
−35.3
−80.6
−20.6
−1.6
−67.7
+27.1
−74.1
−67.8
−49.1
+28.1
−82.7
+31.2
+230.0
+30.7
−22.3
−46.5
−38.9
−17.0
+53.5
−71.7
−280.0
−251.3
−25.3
+11.5
−43.2
+6.0
+50.5
−64.3
−40.1
−102.9
+30.2
−100.6
−3.3
−146.0
−45.1
−129.9
−58.3
−53.5
−36.7
−130.2
−79.7
+47.5
−27.7
−20.5
−35.7
−50.5
+103.7
14.629
14.707
16.276
15.214
15.523
16.072
15.268
15.359
15.497
15.142
14.937
15.464
15.267
15.364
14.911
15.321
15.752
15.355
15.230
14.675
15.719
15.196
15.446
15.591
15.786
15.200
15.197
15.306
15.225
15.632
15.152
14.403
15.372
15.290
15.611
14.839
14.950
15.403
15.031
15.520
15.294
15.548
14.453
16.466
14.505
17.203
10.514
10.530
11.467
11.266
11.331
11.171
11.096
11.217
11.366
11.207
10.975
11.400
11.280
11.201
10.745
11.265
11.084
11.452
11.317
10.677
11.413
11.131
11.463
11.052
11.292
11.217
11.151
11.151
11.245
11.150
10.944
10.165
11.276
11.236
11.461
10.739
10.899
11.489
10.986
11.463
11.306
11.287
10.476
11.381
10.452
11.329
9.642
9.681
10.575
10.375
10.457
10.324
10.219
10.363
10.481
10.384
10.098
10.495
10.444
10.342
9.862
10.430
10.195
10.585
10.468
9.799
10.576
10.264
10.527
10.190
10.422
10.407
10.279
10.287
10.384
10.239
10.029
9.268
10.369
10.402
10.603
9.865
10.085
10.620
10.097
10.652
10.401
10.436
9.641
10.404
9.548
10.340
28
SpT
M4.5
M4.5
M5.0
M4.0
M4.5
M5.5
M4.5
M4.5
M4.5
M4.0
M4.0
M4.0
M4.0
M4.5
M4.5
M4.0
M5.0
M4.0
M4.0
M4.0
M4.5
M4.0
M4.0
M5.0
M5.0
M4.0
M4.0
M4.5
M4.0
M5.0
M4.5
M4.5
M4.0
M4.0
M4.5
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.5
M4.0
M5.5
M4.0
M6.0
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
d
[pc]
22.6
22.8
28.1
39.3
33.0
19.3
29.6
31.3
33.5
38.2
34.4
41.8
39.5
31.1
25.2
39.3
23.6
42.8
40.2
30.0
34.3
36.9
43.0
23.2
25.9
38.4
37.3
30.4
38.9
24.3
27.6
19.3
39.5
38.8
35.0
30.8
33.2
43.5
34.5
43.0
40.0
32.3
27.3
21.2
27.0
16.0
Table A1: (continued).
No.
CMC15
α(J2000)
[deg]
δ(J2000)
[deg]
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
47
48
49
50
51
52
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70
71
72
73
74
75
76
77
78
79
80
81
82
83
84
85
86
87
88
89
90
91
92
93
94
023927.1−033241
024052.6+191342
024508.3−070812
024612.3+351605
024816.8+053705
024857.6−120349
024920.4+435712
025354.0−162453
025407.5+334336
030228.1−325702
030251.6−191150
030303.1−075345
030448.9+223639
030501.9−055430
030602.8−124354
030840.0+135652
031035.9−104607
031312.2+094738
031719.9−011349
031951.9+213828
032000.5+103246
032141.4+140604
032247.1+030953
032409.4+274737
032435.8−322152
032950.3−381200
033114.7−211727
033322.6+284034
033431.6−350103
034049.5−101630
034252.0−191401
034311.6+070216
034422.8+311744
034433.8−200538
034727.8+320955
034729.3+465756
034827.1−194426
035027.9+040645
035056.4+364834
035236.5+173726
035305.9−183550
035306.2−183559
035342.3−252700
035612.8+015139
035624.6−311138
040044.9+135422
040123.5+010649
040424.9−170159
39.863324
40.219441
41.284605
41.551656
42.070027
42.240086
42.335411
43.475193
43.531429
45.617489
45.715005
45.763151
46.203772
46.257944
46.511826
47.166781
47.649974
48.300890
49.333100
49.966441
50.002402
50.422775
50.696445
51.039203
51.149440
52.459672
52.811584
53.344547
53.631987
55.206605
55.717038
55.798499
56.095245
56.140969
56.865842
56.872266
57.113160
57.616485
57.735103
58.152153
58.274938
58.275977
58.426462
59.053519
59.102760
60.187375
60.348318
61.104013
−3.544785
19.228509
−7.136810
35.268297
5.618301
−12.063787
43.953396
−16.414934
33.726735
−32.950697
−19.197224
−7.895873
22.610955
−5.908373
−12.731729
13.948049
−10.768827
9.793979
−1.230419
21.641301
10.546206
14.101272
3.164744
27.793747
−32.364700
−38.200144
−21.290875
28.676385
−35.017582
−10.275070
−19.233850
7.037834
31.295791
−20.093972
32.165543
46.965646
−19.740717
4.112583
36.809681
17.623925
−18.597246
−18.599871
−25.450177
1.860893
−31.194166
13.906316
1.113620
−17.033321
+118.5
+55.5
+38.4
+49.0
+74.1
−96.2
+35.2
+20.5
+98.1
+55.4
+93.3
+21.3
−52.3
−49.8
−15.6
+10.4
+51.2
−6.0
+81.1
+57.3
+48.1
+60.9
+130.3
+28.5
+39.4
+91.3
+87.9
+32.4
+30.0
+94.1
+8.2
−10.8
−40.1
+63.8
+94.0
+9.5
+9.0
+138.7
+21.8
+3.0
+15.5
+18.8
−326.3
+7.0
+39.0
+131.0
+106.7
−64.0
+89.6
−24.9
−43.0
−78.8
−53.8
−34.5
−49.9
+0.1
−72.3
−29.9
−36.9
−76.6
−145.5
+3.4
−16.2
−7.7
−77.5
−24.3
+14.3
−60.4
−29.8
−96.3
−8.7
−63.5
−13.2
−54.4
−94.0
−6.0
−4.8
−46.7
−14.4
−116.6
−42.2
−18.9
−80.3
−10.7
−55.6
+4.6
−47.0
−14.6
+10.8
−5.4
−348.3
−4.0
−119.5
−16.2
−23.0
−198.6
15.675
15.063
14.974
15.003
14.026
15.177
16.028
14.658
15.070
15.347
14.757
15.398
15.508
15.523
15.427
15.270
15.622
15.340
15.032
15.346
15.448
15.015
15.513
15.302
15.244
14.799
14.696
14.739
14.642
15.065
16.722
15.454
15.131
15.314
15.459
15.567
15.340
15.376
15.596
15.262
15.413
15.606
14.600
15.465
14.090
14.209
15.064
15.348
11.332
11.048
10.786
11.070
10.072
10.686
11.480
10.700
10.943
11.299
10.541
11.435
11.219
11.357
11.440
11.300
11.440
11.288
11.089
11.176
11.383
11.109
11.419
11.208
11.294
10.879
10.782
10.797
10.727
10.805
11.445
11.078
11.229
11.318
11.438
11.458
11.197
11.456
11.389
10.984
11.104
11.239
10.473
11.444
10.072
10.260
10.893
11.257
10.451
10.188
9.950
10.205
9.162
9.784
10.579
9.859
10.142
10.387
9.684
10.583
10.326
10.504
10.565
10.448
10.587
10.414
10.233
10.302
10.516
10.260
10.593
10.340
10.397
10.051
9.907
9.896
9.866
9.979
10.539
10.210
10.389
10.485
10.541
10.568
10.270
10.627
10.509
10.120
10.273
10.408
9.518
10.569
9.121
9.344
10.000
10.399
29
SpT
M4.5
M4.0
M4.5
M4.0
M4.0
M5.0
M5.0
M4.0
M4.5
M4.0
M4.5
M4.0
M4.5
M4.5
M4.0
M4.0
M4.5
M4.0
M4.0
M4.5
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.5
M5.5
M4.5
M4.0
M4.0
M4.0
M4.0
M4.5
M4.0
M4.5
M4.5
M4.5
M4.5
M4.5
M4.0
M4.0
M4.0
M4.5
M4.0
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
d
[pc]
33.0
35.5
25.7
35.9
22.7
19.6
28.3
30.3
27.6
39.9
22.9
42.5
31.3
33.4
42.6
39.9
34.7
39.7
36.2
30.7
41.5
36.6
42.2
38.3
39.8
32.9
31.4
31.7
30.7
25.9
21.9
29.4
38.6
40.2
42.5
42.9
31.0
42.9
33.9
28.1
29.7
31.6
22.2
42.7
22.7
24.7
27.0
39.1
Table A1: (continued).
No.
CMC15
α(J2000)
[deg]
δ(J2000)
[deg]
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
95
96
97
98
99
100
101
102
103
104
105
106
107
108
109
110
111
112
113
114
115
116
117
118
119
120
121
122
123
124
125
126
127
128
129
130
131
132
133
134
135
136
137
138
139
140
141
142
040532.1+273313
040546.6+371942
040553.4+053125
040557.0−280946
041436.4+090455
041509.2+190426
041806.4−240626
041840.2−250707
041950.2+292647
042023.3+455228
042044.6+180558
042100.5−355101
042126.5+295247
042137.8−094457
042202.5−133205
042219.9+051112
042320.8+352119
042424.4+361319
042546.2−215359
042703.9+240643
042736.0−231658
042736.4+192645
042741.8+270955
042749.6−332701
042832.0+415723
042832.8+415723
042923.9−293007
042930.1+063516
043224.6+232138
043230.5+232856
043329.6−005939
043352.8+180316
043416.9−252646
043436.6+183625
043555.6+170739
043556.9+235147
043738.7+184208
044044.7+300755
044154.4+091953
044302.4+163156
044405.5+182130
044417.6+203422
044619.2−094702
044714.9−013046
044745.2+302922
044754.8+095357
044840.1−353923
044910.5+134841
61.383956
61.444194
61.472594
61.487905
63.651865
63.788554
64.526708
64.667614
64.959570
65.097472
65.186205
65.252305
65.360491
65.407817
65.510721
65.583265
65.836735
66.101780
66.442679
66.766461
66.900104
66.902048
66.924469
66.956983
67.133465
67.136894
67.349622
67.375728
68.102705
68.127305
68.373588
68.470183
68.570640
68.652659
68.981990
68.987242
69.411407
70.186502
70.476797
70.760202
71.023182
71.073340
71.580112
71.812226
71.938365
71.978396
72.167118
72.294059
27.553836
37.328524
5.523641
−28.162901
9.082129
19.074131
−24.107311
−25.118779
29.446589
45.874576
18.099695
−35.850515
29.879861
−9.749171
−13.534849
5.186738
35.355451
36.222043
−21.899919
24.112219
−23.282981
19.445908
27.165291
−33.450359
41.956653
41.956632
−29.501957
6.588039
23.360630
23.482344
−0.994302
18.054587
−25.446362
18.607071
17.127694
23.863154
18.702396
30.132179
9.331500
16.532258
18.358341
20.572980
−9.784024
−1.512918
30.489710
9.899239
−35.656458
13.811444
+4.7
+96.8
+34.4
+56.7
+73.0
+2.0
−115.3
+152.0
+10.5
+26.0
+20.2
+216.7
+5.1
−38.4
−11.9
+13.4
−72.0
+34.5
+48.3
+18.6
+61.0
+35.0
+8.0
+68.0
−45.0
−102.5
−77.5
+28.9
+4.6
+7.1
+39.8
+16.1
+41.9
+16.3
+14.6
+10.6
−4.1
−101.8
+14.6
+16.4
+14.1
+0.0
+16.9
+37.2
+11.8
+12.8
−66.4
+86.8
−22.8
−78.4
−35.6
−8.4
−3.9
−17.7
−368.1
+132.1
−30.0
+26.7
−39.9
+64.0
−26.1
−64.2
−193.5
−34.6
−36.4
−87.7
−91.7
−25.4
−27.1
+7.0
−14.7
−8.7
−38.9
−40.0
−69.0
−9.9
−23.8
−18.2
−38.3
−15.4
−18.9
−18.9
−19.3
−21.3
−13.6
+38.8
−34.9
−20.7
−25.6
−15.7
−119.5
+10.1
−43.2
−22.8
−133.7
−22.9
15.887
15.273
14.963
15.276
15.438
14.995
15.377
14.416
16.596
14.765
16.129
15.077
15.428
15.009
15.428
16.103
15.136
16.169
15.394
16.144
14.649
15.108
16.254
15.122
15.530
15.305
15.853
15.112
15.072
14.822
15.317
15.332
15.504
14.980
15.274
15.782
15.362
15.528
15.594
14.781
15.163
15.652
15.792
15.233
15.534
15.521
14.753
15.202
11.367
10.915
10.917
11.192
11.374
10.989
10.919
10.366
11.369
10.842
11.194
10.932
10.644
11.093
11.458
11.390
11.123
11.329
11.170
11.343
10.473
11.045
11.246
11.210
11.473
11.388
11.289
11.158
10.831
10.509
11.275
10.865
11.353
10.636
11.078
10.994
11.330
11.463
11.451
10.867
11.074
11.297
11.316
11.261
11.430
11.299
10.521
11.245
10.477
10.042
10.065
10.323
10.528
10.145
10.015
9.476
10.473
9.961
10.313
10.016
9.728
10.176
10.624
10.520
10.262
10.463
10.325
10.362
9.578
10.186
10.356
10.378
10.650
10.571
10.447
10.306
9.899
9.592
10.399
9.932
10.477
9.670
10.141
10.078
10.526
10.620
10.579
9.965
10.148
10.461
10.324
10.454
10.574
10.411
9.652
10.348
30
SpT
M5.0
M4.5
M4.0
M4.0
M4.0
M4.0
M4.5
M4.0
M5.5
M4.0
M5.5
M4.5
M5.0
M4.0
M4.0
M5.0
M4.0
M5.0
M4.5
M5.0
M4.5
M4.0
M5.5
M4.0
M4.0
M4.0
M5.0
M4.0
M4.5
M4.5
M4.0
M4.5
M4.5
M4.5
M4.5
M5.0
M4.0
M4.0
M4.5
M4.0
M4.0
M4.5
M5.0
M4.0
M4.0
M4.5
M4.5
M4.0
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
d
[pc]
26.8
27.2
33.5
38.0
41.3
34.6
27.3
26.0
21.1
32.3
19.5
27.5
19.2
36.3
42.9
27.1
36.8
26.4
30.6
26.5
22.2
35.5
19.9
38.3
43.2
41.6
25.9
37.4
26.2
22.6
39.5
26.6
33.3
24.0
29.4
22.6
40.5
43.0
34.9
32.7
36.0
32.5
26.2
39.2
42.4
32.5
22.7
38.9
Table A1: (continued).
No.
CMC15
α(J2000)
[deg]
δ(J2000)
[deg]
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
143
144
145
146
147
148
149
150
151
152
153
154
155
156
157
158
159
160
161
162
163
164
165
166
167
168
169
170
171
172
173
174
175
176
177
178
179
180
181
182
183
184
185
186
187
188
189
190
044925.7+440541
044957.9+271236
045056.2+121759
045103.9−272548
045218.2+152624
045402.1+082633
045410.4−303636
045455.7−022832
045519.0−321223
045546.3+323903
045757.7+142707
045821.0+105952
045913.2+144838
045928.4+141623
050011.9+055119
050215.7+290323
050324.7+164913
050333.3−382135
050403.8+243534
050440.3+330039
050531.9−191636
050550.0+131455
050806.3+302623
050810.4+080726
050856.9+141317
051051.0−164335
051056.5+130719
051144.8+064940
051146.1−170528
051317.2+273702
051423.6+203153
051429.4+091807
051514.9+195431
051601.2−312445
051630.2−094950
051650.6+022713
051835.4−050435
051844.5+462959
051915.9+065835
051936.9+185951
052126.0−173333
052353.4+324934
052445.6+251444
052454.2+420927
052509.8−133524
052515.3+191713
052632.6−121512
052634.4+001211
72.357240
72.491608
72.734301
72.766440
73.075904
73.509103
73.543394
73.732368
73.829217
73.943187
74.490832
74.587525
74.805385
74.868382
75.049846
75.565558
75.853312
75.888849
76.015932
76.167960
76.383287
76.458435
77.026500
77.043707
77.237286
77.712906
77.735637
77.936702
77.942342
78.321875
78.598548
78.622696
78.812218
79.005052
79.125878
79.211062
79.647896
79.685692
79.816505
79.903817
80.358344
80.972640
81.190002
81.226008
81.290841
81.313984
81.636241
81.643409
44.094860
27.210163
12.299849
−27.430060
15.440120
8.442688
−30.610019
−2.475600
−32.206407
32.651002
14.451959
10.997832
14.810616
14.273289
5.855497
29.056532
16.820550
−38.359909
24.592868
33.010856
−19.276729
13.248661
30.439810
8.124004
14.221436
−16.726581
13.122006
6.828022
−17.091292
27.617223
20.531552
9.302035
19.908846
−31.412702
−9.830598
2.453706
−5.076592
46.499807
6.976581
18.997538
−17.559247
32.826381
25.245714
42.157562
−13.590254
19.286968
−12.253408
0.203068
+75.6
+97.5
−14.7
+30.9
+8.6
+16.8
−18.4
+8.1
+13.1
−7.9
+69.2
+53.4
+8.3
+8.2
+71.4
+2.3
−2.0
−3.8
+22.8
+310.9
+33.4
−2.4
+4.0
+21.0
+20.6
+118.8
+63.7
+121.0
+38.4
−92.6
+59.9
−66.1
−33.4
+39.4
+60.9
+27.1
+10.0
+34.8
+27.1
−12.7
+121.1
+23.4
+19.0
+36.7
+112.9
−10.8
+22.2
−128.4
−27.3
−77.5
−1.7
−3.4
−28.0
−45.3
+126.1
−19.7
+52.7
−0.8
−24.0
−58.5
−28.1
−16.8
+8.2
−18.5
−16.3
+9.0
−51.0
+74.6
−23.2
−19.9
−26.8
−37.2
−9.4
+28.8
−28.0
−65.7
−24.5
−17.5
−35.4
+42.9
−40.2
+0.9
+56.3
−29.2
−71.6
−111.2
−59.5
−30.3
−84.9
−63.2
−70.3
−104.6
−99.8
−29.0
+4.0
−52.7
15.427
14.971
15.012
15.325
16.139
15.304
14.644
15.587
15.162
15.432
15.304
15.313
15.266
14.960
15.193
15.526
15.539
14.805
15.171
16.065
15.588
15.099
15.802
15.403
15.670
15.017
14.788
15.695
14.835
14.641
15.272
14.130
15.139
14.650
15.089
14.907
15.282
13.961
14.609
14.971
15.537
15.785
15.448
15.169
15.606
15.616
14.753
15.156
11.374
11.067
11.105
11.411
11.401
11.349
10.608
11.476
10.683
11.395
11.304
11.300
11.184
10.974
11.236
11.401
11.388
10.863
11.225
11.382
11.478
11.139
11.320
11.439
11.462
11.103
10.800
11.199
10.867
10.732
11.312
10.103
11.030
10.628
11.071
10.742
11.319
9.957
10.698
10.894
11.016
11.385
11.312
11.232
11.227
11.279
10.783
11.133
10.453
10.205
10.275
10.530
10.502
10.516
9.732
10.607
9.814
10.542
10.459
10.437
10.305
10.062
10.367
10.506
10.514
10.014
10.353
10.502
10.622
10.301
10.425
10.526
10.612
10.204
9.923
10.287
9.981
9.909
10.498
9.241
10.219
9.791
10.171
9.873
10.476
9.115
9.871
10.019
10.098
10.513
10.447
10.371
10.329
10.399
9.942
10.292
31
SpT
M4.0
M4.0
M4.0
M4.0
M5.0
M4.0
M4.0
M4.5
M5.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.5
M4.5
M4.0
M4.0
M5.0
M4.5
M4.0
M5.0
M4.0
M4.5
M4.0
M4.0
M5.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.5
M4.0
M4.0
M4.0
M4.0
M5.0
M4.5
M4.5
M4.0
M4.5
M4.5
M4.0
M4.0
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
d
[pc]
41.3
35.9
36.5
42.0
27.3
40.8
29.0
35.3
19.6
41.7
40.0
39.9
37.8
34.4
38.8
34.1
33.9
32.6
38.6
27.0
35.3
37.1
26.3
42.6
35.0
36.5
31.7
24.8
32.7
30.7
40.1
23.0
35.2
29.3
35.9
25.2
40.3
21.5
30.3
33.1
22.8
33.8
32.7
38.7
31.5
32.2
31.5
37.0
Table A1: (continued).
No.
CMC15
α(J2000)
[deg]
δ(J2000)
[deg]
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
191
192
193
194
195
196
197
198
199
200
201
202
203
204
205
206
207
208
209
210
211
212
213
214
215
216
217
218
219
220
221
222
223
224
225
226
227
228
229
230
231
232
233
234
235
236
237
238
052701.9−132749
052706.2−103835
053052.7+321717
053100.2+231218
053151.8−161142
053205.9−030116
053341.7−365444
053506.4−170633
053636.9+130036
053850.8−294056
054109.6+275419
054200.9+181703
054219.7+153936
054328.2−130026
054801.0−250104
054923.8−104256
055128.1−153034
055204.0+355027
055600.4+154600
055613.0+080303
060043.1−004023
060115.4+112053
060126.5−151513
060304.1+360627
060312.3−372243
060536.3+385116
060749.4−262222
061003.7+350004
061042.9+025947
061114.6−003537
061158.0−011717
061436.1+262919
061533.3−101332
061539.6+344331
061616.3+323501
062206.7−163048
062440.7+052045
062607.0−073235
062701.8−310201
062920.1+172516
062959.0+285903
063001.8−192336
063038.1−153904
063050.8+303159
063051.5−065809
063851.1−373217
063944.0−255728
064137.2−372229
81.758148
81.776087
82.719756
82.751140
82.966093
83.024828
83.424098
83.776788
84.153819
84.712048
85.290054
85.503921
85.582180
85.867595
87.004514
87.349170
87.867305
88.017047
89.002073
89.054475
90.179915
90.314406
90.360434
90.767224
90.801367
91.401477
91.955890
92.515678
92.679124
92.811032
92.991916
93.650617
93.889040
93.915084
94.067919
95.527995
96.169585
96.529550
96.757657
97.334010
97.496024
97.507761
97.658921
97.712062
97.714647
99.713223
99.933335
100.405283
−13.463670
−10.643291
32.288139
23.205185
−16.195199
−3.021123
−36.912436
−17.109221
13.010232
−29.682244
27.905481
18.284171
15.660268
−13.007449
−25.017827
−10.715805
−15.509500
35.841031
15.766909
8.050959
−0.673199
11.348141
−15.253699
36.107588
−37.378730
38.854679
−26.372966
35.001150
2.996598
−0.593886
−1.288268
26.488816
−10.225595
34.725368
32.583812
−16.513606
5.345861
−7.543321
−31.033713
17.421307
28.984252
−19.393494
−15.651181
30.533099
−6.969169
−37.538315
−25.957961
−37.374871
−63.0
+97.5
+77.1
+6.8
+39.8
+4.7
+2.0
+480.3
+4.7
+23.6
−13.0
+29.0
+7.6
+137.9
−102.8
+13.7
−233.9
−19.1
−111.5
+6.8
−215.8
−29.0
+20.6
+41.9
+15.0
+5.8
+95.3
+45.7
−92.8
+7.4
+184.7
−48.4
+34.2
−59.9
+3.7
−85.7
−29.5
+0.6
−29.8
+16.9
−103.1
−35.9
+4.9
+39.3
+350.6
−34.3
−21.5
−89.4
−38.5
+41.6
−17.3
−41.9
−13.0
−50.2
+125.3
−92.2
−35.6
−1.0
−122.0
−24.2
−40.3
−169.6
+384.2
−18.7
+352.8
+414.1
+16.5
−28.6
−215.6
−27.1
−9.3
−119.8
−96.5
−53.1
+136.2
−110.5
−22.9
+94.3
−152.6
−99.2
+27.6
−111.1
−68.7
−162.9
−12.2
−19.4
−86.6
−41.6
−69.5
−19.5
+96.2
−48.8
+406.2
+163.8
−96.7
+94.3
16.186
15.110
15.188
14.572
14.756
14.908
14.935
14.209
15.255
15.285
15.621
15.410
14.914
15.453
15.423
14.924
15.367
15.189
15.961
15.538
15.364
15.384
15.414
14.842
14.635
15.032
14.574
14.932
14.325
15.157
15.183
16.049
15.646
15.545
15.180
15.015
14.992
15.296
15.498
16.551
15.384
14.052
15.311
15.474
14.976
14.723
14.844
15.358
11.370
10.994
11.122
10.582
10.757
10.580
10.982
10.178
11.319
11.106
11.331
11.242
10.905
11.235
11.291
10.911
11.426
11.272
11.371
11.482
11.223
11.297
11.466
10.667
10.453
11.104
10.652
10.877
10.363
10.627
11.058
11.300
11.425
11.265
11.231
10.873
11.043
11.371
11.307
11.162
11.305
10.092
11.301
11.378
10.897
10.666
10.902
11.421
10.472
10.103
10.235
9.685
9.875
9.695
10.146
9.295
10.390
10.207
10.400
10.333
10.049
10.343
10.456
10.016
10.555
10.372
10.507
10.596
10.296
10.457
10.616
9.839
9.614
10.268
9.828
10.002
9.473
9.693
10.189
10.429
10.525
10.430
10.370
10.027
10.161
10.556
10.471
10.302
10.447
9.254
10.401
10.504
9.988
9.860
10.055
10.533
32
SpT
M5.0
M4.5
M4.0
M4.0
M4.0
M4.5
M4.0
M4.0
M4.0
M4.5
M4.5
M4.5
M4.0
M4.5
M4.5
M4.0
M4.0
M4.0
M5.0
M4.0
M4.5
M4.0
M4.0
M4.5
M4.5
M4.0
M4.0
M4.0
M4.0
M5.0
M4.5
M5.0
M4.5
M4.5
M4.0
M4.5
M4.0
M4.0
M4.5
M6.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
d
[pc]
26.9
28.3
36.8
28.7
31.1
23.3
34.5
23.8
40.3
29.7
33.0
31.7
33.3
31.6
32.4
33.4
42.3
39.4
26.9
43.4
31.4
39.9
43.1
24.3
22.0
36.5
29.6
32.8
25.9
19.1
29.1
26.0
34.5
32.0
38.7
26.7
35.5
41.2
32.6
14.8
40.0
22.9
39.9
41.4
33.2
29.8
33.2
42.2
Table A1: (continued).
No.
CMC15
α(J2000)
[deg]
δ(J2000)
[deg]
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
239
240
241
242
243
244
245
246
247
248
249
250
251
252
253
254
255
256
257
258
259
260
261
262
263
264
265
266
267
268
269
270
271
272
273
274
275
276
277
278
279
280
281
282
283
284
285
286
064142.8+122643
064149.3+014923
064547.8−191831
064920.4+065519
065120.2+013458
065150.8−303337
065211.2−384734
065301.8−092640
065549.8−084215
065649.4+132933
070512.0−100752
071633.3+084848
071733.0+104849
072055.3+442721
072151.1+211454
072239.0+321328
072305.1+462742
072400.7−263610
072417.3+183847
072420.1+382053
073001.9−283102
073100.2−291723
073227.9−254303
073255.1−200314
073655.1+364420
074508.3−070128
074610.7−185903
074656.4+430415
075313.5−101219
075405.3+022344
075529.8+255635
075705.0−222643
075831.9−293412
080259.4−163929
081202.5+070932
082000.3−231826
082346.6−243404
082508.6−222513
082558.9−261135
083214.0+091027
083505.4+423032
083538.4+162856
083740.5+482303
084040.8−383238
084247.0−245827
084615.3+040638
084900.6+285951
085443.9−091103
100.428683
100.455513
101.449367
102.335219
102.834184
102.961840
103.046689
103.257856
103.957619
104.205983
106.300107
109.138890
109.387808
110.230582
110.463206
110.662768
110.771562
111.002945
111.072163
111.083997
112.508195
112.751001
113.116285
113.229914
114.229620
116.284850
116.544733
116.735015
118.306376
118.522269
118.874373
119.271122
119.633038
120.747535
123.010691
125.001628
125.944247
126.285977
126.495481
128.058663
128.772606
128.910324
129.418750
130.170005
130.696087
131.563831
132.252532
133.683152
12.445480
1.823119
−19.308711
6.922153
1.582806
−30.560439
−38.793027
−9.444687
−8.704259
13.492616
−10.131188
8.813479
10.813882
44.455922
21.248364
32.224459
46.461744
−26.602849
18.646593
38.348266
−28.517404
−29.289856
−25.717775
−20.054103
36.738973
−7.024495
−18.984391
43.071048
−10.205307
2.395830
25.943137
−22.445296
−29.570096
−16.658249
7.159164
−23.307433
−24.567797
−22.420361
−26.193244
9.174312
42.508916
16.482464
48.384399
−38.543923
−24.974435
4.110666
28.997507
−9.184197
+12.6
−26.0
+19.2
−51.3
−140.1
−5.9
−93.8
−14.8
−4.8
−35.3
+123.7
−2.0
−39.8
−12.4
+25.9
−16.8
−23.7
−101.6
−54.9
+33.7
−150.5
−81.1
−153.0
−191.9
−83.5
+163.4
−107.8
−16.3
+146.3
+26.3
+39.8
+5.1
+47.0
+27.3
+77.5
−57.5
+46.6
−99.7
−153.5
−98.2
−2.0
+8.9
−8.9
+91.6
−74.4
+16.4
−92.4
+21.8
−21.7
+36.6
+38.9
−32.1
+12.0
−1.0
+6.9
+66.7
+5.3
−46.8
+77.5
−25.8
−25.6
+0.7
−77.5
−26.8
−105.1
+100.0
−47.6
−49.6
+92.4
−14.2
+59.6
−146.4
−126.1
+119.5
+111.7
−46.0
−360.5
−3.8
−50.7
−83.5
+75.6
+30.0
+74.4
+17.1
−21.7
+18.2
+100.5
+22.2
+22.4
−10.3
−124.6
−62.8
−89.1
−99.9
−71.9
+3.0
14.405
15.248
14.816
15.396
15.828
15.078
15.351
16.019
15.405
15.806
14.369
15.043
15.403
15.620
14.523
15.326
15.577
15.296
14.563
14.388
14.979
15.646
15.316
15.656
15.379
15.051
15.914
16.221
15.870
14.922
15.412
14.808
14.712
15.561
14.546
15.321
15.032
14.628
15.458
15.191
15.522
15.203
15.670
14.087
14.407
14.268
15.473
15.382
10.227
11.316
10.890
11.444
11.439
10.799
11.275
11.415
11.406
11.444
10.196
11.123
11.477
11.470
10.505
11.264
11.466
11.299
10.591
10.408
10.634
11.350
11.012
11.188
11.217
11.122
11.402
11.411
11.410
10.966
11.401
10.785
10.693
11.468
10.536
11.358
11.013
10.548
11.350
11.138
11.288
11.281
11.460
9.790
10.348
10.244
11.253
11.449
9.358
10.451
9.999
10.549
10.524
9.930
10.277
10.481
10.580
10.568
9.275
10.241
10.624
10.581
9.640
10.343
10.530
10.400
9.739
9.559
9.747
10.488
10.135
10.310
10.344
10.303
10.482
10.573
10.601
10.137
10.555
9.880
9.740
10.542
9.688
10.513
10.154
9.671
10.461
10.250
10.433
10.443
10.536
8.868
9.503
9.320
10.387
10.567
33
SpT
M4.5
M4.0
M4.0
M4.0
M4.5
M4.5
M4.0
M5.0
M4.0
M4.5
M4.5
M4.0
M4.0
M4.5
M4.0
M4.0
M4.5
M4.0
M4.0
M4.0
M4.5
M4.5
M4.5
M4.5
M4.5
M4.0
M5.0
M5.0
M4.5
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.5
M4.0
M4.5
M4.5
M4.0
M4.0
M4.5
M4.0
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
d
[pc]
19.8
40.2
33.0
42.7
34.7
25.8
39.5
27.4
41.9
34.8
19.6
36.8
43.3
35.2
27.7
39.3
35.1
39.9
28.8
26.5
23.9
33.3
28.5
30.9
31.3
36.8
27.3
27.4
34.2
34.2
41.8
31.5
30.2
43.1
28.1
41.0
35.0
28.2
40.8
37.0
32.3
39.6
35.0
16.2
25.7
24.5
31.8
42.7
Table A1: (continued).
No.
CMC15
α(J2000)
[deg]
δ(J2000)
[deg]
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
287
288
289
290
291
292
293
294
295
296
297
298
299
300
301
302
303
304
305
306
307
308
309
310
311
312
313
314
315
316
317
318
319
320
321
322
323
324
325
326
327
328
329
330
331
332
333
334
085601.3−103449
085634.5−311758
085831.2+401553
090034.9−075758
090101.4−110159
090351.2+221445
090358.7+402238
090756.7+374324
090913.2−021611
090934.7−365452
091321.8−292716
091624.4−245529
091957.2−062535
092311.4−352313
092312.2−314522
092327.7−190931
093934.1−173555
094319.7−333506
094518.3−094024
095747.7−061108
100003.6+331305
100009.7+064703
100410.2−032934
100550.7+350813
100626.9+412656
100754.7−201429
101107.6−053328
101114.0−272512
101114.1−272526
101206.6+181841
101331.8+160620
102038.0−061534
102128.0+250722
102207.9+023408
102345.3−132547
102428.8+175015
102809.5−231457
102824.8−395923
103850.2−205424
103954.8+183904
104306.8+152631
104834.6−151204
104909.7−010812
105045.0−073629
105423.0−150708
105850.4−234620
110058.3+480334
110721.9−265344
134.005657
134.143837
134.630216
135.145507
135.256163
135.963413
135.994935
136.986575
137.305390
137.394931
138.341060
139.101925
139.988655
140.797866
140.801087
140.865804
144.892499
145.832085
146.326308
149.448754
150.015098
150.040819
151.042895
151.461660
151.612295
151.978132
152.781913
152.808427
152.809126
153.027653
153.382770
155.158450
155.366848
155.533091
155.938952
156.120100
157.039902
157.103725
159.709328
159.978656
160.778514
162.144335
162.290428
162.687630
163.595843
164.710387
165.243162
166.841365
−10.580546
−31.299563
40.264730
−7.966126
−11.033323
22.245921
40.377370
37.723342
−2.269956
−36.914529
−29.454503
−24.924977
−6.426558
−35.387092
−31.756257
−19.158623
−17.598659
−33.585271
−9.673570
−6.185733
33.218183
6.784411
−3.493011
35.137111
41.449128
−20.241622
−5.558051
−27.420164
−27.423990
18.311619
16.105591
−6.259539
25.123014
2.568929
−13.429823
17.837636
−23.249206
−39.989749
−20.906869
18.651304
15.442066
−15.201147
−1.136771
−7.608272
−15.119003
−23.772458
48.059550
−26.895830
−26.5
−162.2
−1.6
+147.3
−33.8
−41.7
−29.5
+5.2
+90.6
−97.1
−7.5
−34.3
−144.6
−55.4
−109.8
−11.3
−24.7
−100.6
−85.1
+54.8
−48.5
−356.9
−101.2
+151.0
+28.5
−25.1
−352.2
−20.6
−15.0
+14.2
−25.5
+119.9
−13.4
+40.8
−129.8
−84.9
+14.2
−152.3
−105.4
+41.2
−87.7
+0.7
−5.8
−77.6
−102.1
−99.7
−37.9
+70.1
−18.2
+61.1
−105.6
−43.4
−181.0
+0.7
−155.4
+59.0
+375.1
+63.8
+4.8
−9.1
−67.3
−23.9
+191.0
−158.8
−47.8
+2.3
−64.2
−9.3
−135.4
+212.7
+13.1
+149.6
+14.1
−120.5
−261.8
+16.4
+17.3
−79.9
−10.4
−108.5
−77.4
−112.0
+37.4
−11.1
−148.5
+13.3
+45.8
−151.0
−48.9
+21.2
−17.9
−114.0
−71.0
−18.4
−85.8
−30.9
15.253
15.509
15.158
15.145
15.232
15.168
15.777
15.290
15.229
15.449
14.116
15.372
16.007
14.306
14.895
15.448
15.340
15.745
15.140
15.311
15.632
14.912
15.271
15.143
15.445
16.043
15.206
15.391
15.297
15.685
15.500
14.885
15.482
14.651
14.663
15.581
15.560
14.886
15.332
15.244
15.489
14.048
15.609
15.454
15.567
14.861
14.645
15.474
11.290
11.445
11.158
10.968
11.321
11.097
11.497
11.258
11.175
11.382
10.063
11.434
11.232
10.404
10.978
11.395
11.410
11.473
10.945
11.185
11.493
10.929
11.343
11.196
11.050
11.167
11.203
11.477
10.956
11.272
11.475
10.844
11.275
10.711
10.620
11.480
11.335
10.867
11.363
11.267
11.468
9.986
11.120
11.398
11.097
10.302
10.699
11.485
10.441
10.583
10.217
10.160
10.449
10.274
10.582
10.446
10.321
10.490
9.183
10.597
10.296
9.584
10.172
10.464
10.511
10.588
10.030
10.313
10.658
10.089
10.516
10.326
10.215
10.221
10.356
10.675
10.120
10.388
10.603
9.987
10.428
9.871
9.763
10.622
10.424
10.025
10.548
10.389
10.652
9.139
10.224
10.439
10.256
9.430
9.780
10.646
34
SpT
M4.0
M4.0
M4.0
M4.5
M4.0
M4.0
M4.5
M4.0
M4.0
M4.0
M4.0
M4.0
M5.0
M4.0
M4.0
M4.0
M4.0
M4.5
M4.5
M4.5
M4.5
M4.0
M4.0
M4.0
M4.5
M5.5
M4.0
M4.0
M4.5
M4.5
M4.0
M4.0
M4.5
M4.0
M4.0
M4.0
M4.5
M4.0
M4.0
M4.0
M4.0
M4.0
M5.0
M4.0
M5.0
M5.0
M4.0
M4.0
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
d
[pc]
39.7
42.7
37.4
27.9
40.3
36.4
35.6
39.1
37.7
41.5
22.6
42.5
25.2
26.4
34.4
41.7
42.0
35.2
27.6
30.8
35.5
33.6
40.7
38.0
29.0
19.2
38.2
43.3
27.8
32.1
43.3
32.4
32.2
30.4
29.2
43.4
33.1
32.7
41.1
39.3
43.1
21.8
24.0
41.8
23.7
16.4
30.3
43.5
Table A1: (continued).
No.
CMC15
α(J2000)
[deg]
δ(J2000)
[deg]
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
335
336
337
338
339
340
341
342
343
344
345
346
347
348
349
350
351
352
353
354
355
356
357
358
359
360
361
362
363
364
365
366
367
368
369
370
371
372
373
374
375
376
377
378
379
380
381
382
111015.5−241143
111548.1+274616
111551.4−345011
111618.6−254923
112055.8+164030
112905.6+360701
113049.8+153357
113208.4−131922
113343.4+464747
113622.0−235628
113928.8−065214
114113.5−160151
114914.6+300145
115102.3−361146
115637.3+264602
115858.1−274054
120056.8−375918
120237.9−332840
120254.1+414810
120532.3+425502
121004.4+124409
121408.0+471603
122150.1+463244
122409.6+035604
122607.0−002205
123015.8−312404
123116.2−152950
123244.3−153055
123726.2−352717
123745.5+384232
123901.6+130955
124046.1−302629
124112.3−273210
124358.7−161434
125348.6−084216
125657.8+381608
125812.6+462952
130428.0−084530
130618.1−342857
130619.9+133009
130728.9+332508
130733.7+111303
131640.5−085825
131708.2−335443
131841.5−314307
132132.7−253615
132554.4−023214
132748.2−294107
167.564990
168.950525
168.964278
169.077540
170.232621
172.273440
172.707728
173.035220
173.430903
174.091695
174.870010
175.306569
177.310872
177.759837
179.155469
179.742445
180.236732
180.658107
180.725451
181.384689
182.518501
183.533728
185.459052
186.040350
186.529188
187.566081
187.817644
188.184935
189.359203
189.439706
189.756750
190.192160
190.301463
190.994634
193.452573
194.240957
194.552663
196.116872
196.575651
196.583125
196.870766
196.890585
199.168795
199.284377
199.673108
200.386255
201.477046
201.951087
−24.195330
27.771116
−34.836469
−25.823063
16.675170
36.117067
15.565974
−13.322793
46.796482
−23.941359
−6.870793
−16.030892
30.029391
−36.196160
26.767284
−27.681881
−37.988578
−33.477899
41.802814
42.917311
12.736087
47.267658
46.545719
3.934561
−0.368190
−31.401337
−15.497318
−15.515476
−35.454808
38.708992
13.165286
−30.441611
−27.536111
−16.242935
−8.704644
38.268998
46.498007
−8.758414
−34.482531
13.502628
33.418932
11.217571
−8.973883
−33.912146
−31.718829
−25.604329
−2.537406
−29.685502
−183.0
+95.0
−53.7
−105.8
+39.3
+16.9
−64.9
−130.1
−100.1
−130.4
−47.5
−77.6
+60.5
−147.9
−140.5
−93.1
+110.0
−75.6
+2.5
+15.4
−34.4
−138.2
+90.7
−19.2
−157.8
−112.0
+28.0
−180.2
+59.2
+25.4
−66.1
+145.9
−109.4
−429.2
−266.2
−3.5
−95.6
−119.2
−21.6
−19.5
+66.4
+58.3
−112.8
−99.1
+15.6
−68.1
−160.6
+83.4
+3.3
−31.2
+17.5
−240.1
+11.4
−94.7
−112.7
+37.6
−79.6
+42.7
−1.8
+124.9
+34.1
−45.9
+7.8
−51.2
−69.2
−12.9
−39.0
+21.9
−30.3
−74.3
−9.7
−135.7
+14.7
−12.8
−108.5
−176.4
−28.6
−21.9
−22.6
−95.4
−93.7
+82.3
−170.2
−5.6
+103.2
−25.4
−10.3
−115.6
+25.1
−2.8
−142.8
+5.3
−57.0
−7.8
+1.6
−96.1
14.814
16.735
15.090
14.674
15.253
14.938
15.646
15.170
15.496
15.387
15.296
15.862
15.533
15.528
15.080
15.615
15.480
14.921
15.381
15.283
14.374
15.095
16.584
15.714
15.459
16.260
15.063
16.154
15.923
15.325
15.413
14.699
14.841
14.113
15.215
14.533
15.465
15.755
15.112
14.969
15.954
15.216
13.954
15.686
15.205
15.097
15.644
14.955
10.868
11.284
11.160
10.650
11.187
10.932
11.094
10.913
11.459
11.327
11.360
11.442
11.358
11.206
11.130
11.487
11.121
10.686
11.340
11.120
10.311
11.172
11.259
11.378
11.395
11.382
10.987
11.384
11.262
11.340
11.465
10.500
10.907
9.777
10.737
9.769
11.450
11.483
10.503
10.757
11.432
11.162
10.043
11.423
11.175
11.167
11.270
10.987
9.973
10.324
10.273
9.693
10.307
10.059
10.184
10.040
10.597
10.431
10.549
10.569
10.446
10.320
10.289
10.668
10.239
9.847
10.474
10.268
9.449
10.315
10.286
10.453
10.537
10.391
10.096
10.462
10.381
10.494
10.663
9.618
10.054
8.896
9.855
8.785
10.616
10.568
9.632
9.891
10.606
10.279
9.199
10.554
10.336
10.309
10.417
10.154
35
SpT
M4.0
M6.0
M4.0
M4.0
M4.0
M4.0
M5.0
M4.5
M4.0
M4.0
M4.0
M4.5
M4.5
M4.5
M4.0
M4.5
M4.5
M4.5
M4.0
M4.5
M4.0
M4.0
M6.0
M4.5
M4.0
M5.5
M4.0
M5.0
M5.0
M4.0
M4.0
M4.5
M4.0
M4.5
M5.0
M5.0
M4.0
M4.5
M5.0
M4.5
M5.0
M4.0
M4.0
M4.5
M4.0
M4.0
M4.5
M4.0
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
d
[pc]
32.7
15.7
37.4
29.6
37.9
33.7
23.7
27.2
42.9
40.4
41.0
34.7
33.4
31.1
36.9
35.5
30.0
24.5
40.7
29.9
25.3
37.6
15.5
33.7
41.7
21.2
34.6
27.1
25.6
40.7
43.1
22.5
33.3
16.1
20.1
12.9
42.8
35.4
18.0
25.3
27.7
37.5
22.4
34.4
37.7
37.5
32.1
34.6
Table A1: (continued).
No.
CMC15
α(J2000)
[deg]
δ(J2000)
[deg]
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
383
384
385
386
387
388
389
390
391
392
393
394
395
396
397
398
399
400
401
402
403
404
405
406
407
408
409
410
411
412
413
414
415
416
417
418
419
420
421
422
423
424
425
426
427
428
429
430
132939.8+055052
133226.9−385147
133255.6−291620
133356.0−075822
133531.2−015930
133559.6+402146
133823.0−172423
134058.6−303109
134513.1−311328
135104.6+492409
135207.2+462605
135518.3−175345
135657.6+273100
135753.7+230846
135821.6−004626
135850.2−331520
140101.7+174317
140246.4+130327
140637.5−090454
141147.8−365227
141230.2+305935
141443.0+261639
142222.8+082422
142225.0+135642
142742.1−003851
142812.6+160429
143011.6−073139
143110.2−212858
143202.4−103321
143204.8−332626
143743.1+261656
143856.8−092801
143915.2−352711
144109.1−272717
144126.0+244150
144414.7−365755
144456.2+235103
144507.1−352634
144509.3−331338
144557.5+145812
144624.4+150201
144625.5−373027
144644.2−365905
144713.8−321739
144738.1+035309
144739.2+011634
145232.8−094547
145313.2+155254
202.416177
203.112302
203.232082
203.483684
203.880003
203.998738
204.596166
205.244496
206.304960
207.769271
208.030360
208.826404
209.240353
209.473999
209.590039
209.709499
210.257202
210.693620
211.656354
212.949400
213.125997
213.679542
215.595261
215.604568
216.925761
217.052745
217.548396
217.792665
218.010270
218.020320
219.429894
219.736785
219.813537
220.288245
220.358650
221.061488
221.234227
221.279730
221.288767
221.489640
221.601930
221.606480
221.684325
221.807526
221.908914
221.913689
223.136845
223.305352
5.847997
−38.863307
−29.272268
−7.972936
−1.991726
40.362795
−17.406506
−30.519359
−31.224631
49.402599
46.434726
−17.895864
27.516934
23.146156
−0.774022
−33.255801
17.721420
13.057614
−9.081935
−36.874289
30.993139
26.277712
8.406223
13.945210
−0.647571
16.074889
−7.527766
−21.482798
−10.556039
−33.440672
26.282294
−9.467033
−35.453274
−27.454868
24.697308
−36.965306
23.851013
−35.442787
−33.227433
14.970105
15.033698
−37.507681
−36.984740
−32.294236
3.886045
1.276251
−9.763270
15.881778
+99.9
−125.8
−232.8
+70.8
−22.7
+34.0
−14.0
+99.2
−163.2
−22.9
+114.2
−76.0
−33.1
−86.4
−82.2
−34.8
+46.4
−17.8
+0.6
−21.9
−106.5
+51.8
+39.3
−62.6
−27.5
−38.8
−195.6
+121.3
−158.6
+166.3
−21.3
−106.9
−35.7
+13.4
+60.1
−8.5
+67.6
−130.8
−20.4
−38.3
−51.0
−39.8
−11.9
+596.3
+12.0
−135.2
−249.5
+4.0
−101.0
−23.5
−31.8
−30.5
+41.7
+27.5
−58.9
−71.2
−17.4
−24.0
−36.9
−11.5
−150.9
−29.3
−74.0
−27.0
+48.2
−9.2
−134.2
−29.6
+21.5
−3.4
−119.7
−54.8
−37.1
+33.1
+165.9
−26.6
−15.2
−86.7
−143.0
−42.9
−32.4
−7.8
−20.8
+9.1
−71.9
−13.3
−27.2
−37.2
+42.6
+41.8
−21.4
−478.5
−53.2
+7.9
−199.0
−95.2
15.291
15.342
14.953
15.880
15.643
15.837
15.269
15.459
15.790
15.009
15.225
15.801
15.807
15.851
15.694
15.285
15.262
15.317
15.102
15.522
15.425
15.380
15.340
15.666
15.320
15.065
15.107
16.015
15.608
14.515
15.494
15.250
15.402
15.205
15.386
14.926
15.140
15.673
15.620
15.595
15.267
15.251
15.387
15.649
16.025
15.168
15.617
15.161
11.284
11.276
10.569
11.456
11.442
11.210
11.349
11.456
11.473
11.096
11.152
11.353
11.238
11.425
10.808
11.265
11.110
11.414
11.050
11.483
11.438
11.447
11.086
11.268
11.358
11.013
11.184
11.423
11.489
10.371
11.406
11.026
11.388
11.275
11.466
10.937
11.021
11.419
11.449
11.383
11.364
11.281
11.430
11.487
11.480
11.113
11.325
11.240
10.450
10.368
9.676
10.554
10.605
10.298
10.520
10.609
10.596
10.203
10.279
10.506
10.303
10.596
9.941
10.407
10.302
10.576
10.233
10.615
10.595
10.633
10.170
10.340
10.510
10.143
10.370
10.532
10.604
9.534
10.474
10.162
10.583
10.442
10.654
10.056
10.183
10.493
10.609
10.542
10.490
10.373
10.520
10.587
10.611
10.255
10.508
10.395
36
SpT
M4.0
M4.0
M4.5
M4.5
M4.5
M5.0
M4.0
M4.0
M4.5
M4.0
M4.0
M4.5
M5.0
M4.5
M5.5
M4.0
M4.5
M4.0
M4.0
M4.0
M4.0
M4.0
M4.5
M4.5
M4.0
M4.0
M4.0
M5.0
M4.5
M4.5
M4.0
M4.5
M4.0
M4.0
M4.0
M4.0
M4.5
M4.5
M4.5
M4.5
M4.0
M4.0
M4.0
M4.5
M5.0
M4.0
M4.5
M4.0
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
d
[pc]
39.6
39.5
23.2
34.9
34.7
25.0
40.8
42.9
35.2
36.3
37.3
33.3
25.3
34.5
16.3
39.3
29.8
42.1
35.6
43.4
42.5
42.7
29.5
32.1
41.0
35.0
37.8
27.5
35.5
21.2
41.9
28.7
41.6
39.5
43.1
33.8
28.6
34.4
34.8
33.8
41.1
39.6
42.4
35.5
28.3
36.6
32.9
38.8
Table A1: (continued).
No.
CMC15
α(J2000)
[deg]
δ(J2000)
[deg]
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
431
432
433
434
435
436
437
438
439
440
441
442
443
444
445
446
447
448
449
450
451
452
453
454
455
456
457
458
459
460
461
462
463
464
465
466
467
468
469
470
471
472
473
474
475
476
477
478
145536.1−033223
145937.7−230645
150113.5−093326
150455.8−261329
150516.9−381412
150731.9−125059
150744.3−022541
150950.9+150250
151239.6−163101
151250.7−390119
151355.4−394114
151412.0−374406
151534.7−252701
151602.2−323202
151607.9−242008
151634.8−350030
151750.6+114335
151945.6−022359
152012.7−355925
152045.4−075614
152229.6−230938
152448.3−311908
152452.4+284701
152502.3+060443
152559.7+114607
152623.3+330529
152726.4−334356
152732.4−023623
152756.4−193750
152806.3−325801
152809.0−125847
152817.8−211751
152857.5−371427
153013.7−140144
153021.8−135846
153109.3−165430
153116.7+344126
153122.1−031900
153139.0−104244
153140.8+021042
153159.7−351755
153258.1−044534
153307.1−092507
153348.6−291126
153444.6−280026
153454.8−072143
153510.7−384130
153546.3−341317
223.900668
224.907192
225.306343
226.232620
226.320446
226.882966
226.934892
227.462126
228.165320
228.211486
228.481247
228.550305
228.894895
229.009216
229.032988
229.145345
229.461005
229.940033
230.053122
230.189264
230.623548
231.201421
231.218570
231.259713
231.499075
231.597402
231.860179
231.885139
231.985047
232.026497
232.037784
232.074503
232.239904
232.557286
232.590995
232.788754
232.819720
232.842364
232.912756
232.920411
232.998753
233.242408
233.279663
233.452500
233.686218
233.728474
233.794599
233.943333
−3.539994
−23.112741
−9.557320
−26.224777
−38.236748
−12.849841
−2.428311
15.047394
−16.517036
−39.021954
−39.687272
−37.735131
−25.450461
−32.534153
−24.335621
−35.008365
11.726459
−2.399934
−35.990471
−7.937260
−23.160749
−31.318930
28.783760
6.078775
11.768828
33.091575
−33.732308
−2.606485
−19.630679
−32.966964
−12.979782
−21.297696
−37.240904
−14.028960
−13.979665
−16.908592
34.690684
−3.316854
−10.712242
2.178397
−35.298726
−4.759701
−9.418887
−29.190765
−28.007253
−7.362144
−38.691681
−34.221503
−334.0
−66.6
−90.1
−29.1
−52.7
−108.8
+47.8
−35.4
−108.8
−83.6
−75.9
−19.2
−25.6
−13.9
−25.2
−18.1
−27.1
+51.2
+64.1
−69.3
−20.5
−23.6
+11.1
+60.5
−136.6
−116.2
−19.0
+47.4
+9.2
−28.2
−28.7
+260.6
+82.1
−46.3
−163.0
−17.6
−101.3
−103.4
+127.8
+14.6
+16.6
−20.0
−75.7
+8.3
−37.2
+1.4
−18.1
−17.5
+68.7
−75.8
−89.8
−32.7
−11.4
−5.1
−40.0
−97.8
−15.1
−112.9
−100.8
−22.6
−31.3
−11.0
−27.4
−28.7
−21.9
−149.6
−239.0
−70.9
−26.3
−27.7
+6.3
−24.1
−40.6
−69.4
−33.3
−5.6
−3.1
−24.0
−24.4
−248.4
−129.2
−8.5
−385.8
−33.0
+39.8
+17.9
−16.6
−529.2
−127.3
−16.2
−72.3
−60.2
−41.9
−14.6
−27.0
−18.7
15.196
15.669
15.515
15.545
14.838
15.851
14.600
16.435
14.803
14.550
15.252
15.434
15.649
15.356
14.982
14.908
15.402
15.659
16.523
14.481
15.347
15.657
15.519
14.969
15.223
15.915
15.389
15.404
15.474
15.456
15.351
15.688
15.097
16.178
15.389
16.005
14.640
14.966
15.116
15.680
15.470
16.098
15.068
16.344
14.260
15.097
14.999
15.471
11.067
11.495
11.195
11.485
10.866
11.475
10.697
11.450
10.793
10.351
10.491
11.325
11.230
11.427
10.952
10.983
11.387
11.350
11.472
10.346
11.354
11.456
11.473
11.050
11.242
11.383
11.385
11.394
11.375
11.330
10.921
11.487
11.167
11.243
11.445
11.223
10.732
11.033
11.156
11.427
11.337
11.311
11.129
11.105
10.332
10.862
11.087
11.456
10.214
10.609
10.340
10.620
9.968
10.592
9.891
10.525
9.880
9.422
9.587
10.489
10.358
10.547
10.027
10.108
10.507
10.511
10.639
9.435
10.431
10.610
10.610
10.192
10.413
10.520
10.504
10.523
10.471
10.499
10.042
10.630
10.321
10.396
10.576
10.371
9.881
10.199
10.334
10.523
10.474
10.418
10.325
10.272
9.422
9.988
10.222
10.630
37
SpT
M4.5
M4.5
M4.5
M4.0
M4.0
M4.5
M4.0
M5.5
M4.0
M4.5
M5.0
M4.0
M4.5
M4.0
M4.0
M4.0
M4.0
M4.5
M5.5
M4.5
M4.0
M4.5
M4.0
M4.0
M4.0
M5.0
M4.0
M4.0
M4.0
M4.5
M4.5
M4.5
M4.0
M5.5
M4.0
M5.0
M4.0
M4.0
M4.0
M4.5
M4.5
M5.0
M4.0
M5.5
M4.0
M4.5
M4.0
M4.0
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
d
[pc]
29.2
35.6
31.0
43.5
32.7
35.3
30.2
21.9
31.6
21.0
17.9
40.4
31.5
42.3
34.0
34.5
41.5
33.3
22.1
21.0
40.9
34.9
43.2
35.6
38.9
27.0
41.5
41.7
41.3
33.0
27.3
35.5
37.5
19.9
42.7
25.1
30.7
35.3
37.4
34.5
33.1
26.2
36.9
18.7
25.6
26.6
36.2
42.9
Table A1: (continued).
No.
CMC15
α(J2000)
[deg]
δ(J2000)
[deg]
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
479
480
481
482
483
484
485
486
487
488
489
490
491
492
493
494
495
496
497
498
499
500
501
502
503
504
505
506
507
508
509
510
511
512
513
514
515
516
517
518
519
520
521
522
523
524
525
526
153654.4−292857
153758.2+054724
153830.8−314458
153845.2+380413
154007.7+103318
154018.0−041211
154316.1−251902
154541.8−051531
154609.7−344828
154707.7+153409
154734.9−275342
154736.7−312642
154833.6+080302
154910.6−352307
154919.7−225729
155105.4−285623
155233.4−231119
155358.7−231543
155443.7+001422
155450.4−052147
155500.2−234508
155501.9−275453
155518.9+314650
155556.6−371615
155603.4−364355
155612.1−235407
155625.1−201615
155625.2−262828
155701.0−150115
155703.6−230448
155711.6−362801
155749.3+124516
155758.3−340548
155803.1−343305
155924.1−211631
155938.0−260323
160357.6−175510
160424.4−364618
160607.2−022052
160616.4−361800
160638.0−272755
160734.9−273616
160758.5−062108
160826.9+171843
160838.6+253452
160842.5−273330
160849.8+002455
160856.9−283557
234.226860
234.492884
234.628379
234.688581
235.032164
235.075225
235.817183
236.424435
236.540590
236.782214
236.895674
236.902963
237.140095
237.294439
237.332289
237.772565
238.139415
238.494923
238.682249
238.710041
238.751016
238.758144
238.828874
238.985972
239.014214
239.050671
239.104605
239.105208
239.254190
239.265362
239.298614
239.455532
239.492998
239.512957
239.850619
239.908624
240.990094
241.101780
241.530128
241.568670
241.658473
241.895668
241.993768
242.112138
242.161041
242.177308
242.207729
242.237290
−29.482671
5.790197
−31.749488
38.070438
10.555094
−4.203163
−25.317430
−5.258766
−34.807847
15.569352
−27.895163
−31.445083
8.050729
−35.385380
−22.958251
−28.939854
−23.188724
−23.262172
0.239630
−5.363172
−23.752396
−27.914793
31.780804
−37.270898
−36.732111
−23.902161
−20.271101
−26.474639
−15.021038
−23.080155
−36.467177
12.754595
−34.096919
−34.551461
−21.275481
−26.056565
−17.919564
−36.771940
−2.347796
−36.300042
−27.465414
−27.604638
−6.352357
17.312193
25.581184
−27.558413
0.415410
−28.599321
−78.8
+3.9
−23.1
−70.7
−0.4
−16.8
−8.6
−15.8
−64.3
−68.2
+102.8
−38.7
−5.0
−18.6
−12.8
−15.6
−25.5
−10.9
−76.3
+145.7
−37.2
−18.1
−45.6
−9.9
−30.0
−19.7
−13.4
−27.6
+25.3
−12.1
−20.8
−19.9
−144.8
+9.5
−15.8
−72.2
−2.6
−25.9
−173.4
−1.9
−8.4
−14.7
−211.0
+33.6
−65.9
−25.7
−94.7
−14.6
−23.7
−68.0
−27.1
−14.8
−141.3
−20.9
−20.4
−25.4
+60.0
−28.9
+7.0
−51.0
−111.9
−28.2
−30.3
−25.8
−13.1
−17.0
−83.7
−119.9
−39.1
−26.5
+26.2
−25.8
−40.4
−28.8
−24.1
−32.9
−18.9
−22.8
−45.4
+8.9
−52.4
−26.8
−29.5
−10.0
−14.3
−22.4
+205.8
−62.9
−13.7
−22.7
+45.2
−27.2
−82.7
−28.6
+16.4
−23.2
15.528
15.874
15.632
15.376
15.266
15.808
16.053
14.562
15.283
15.592
16.010
15.034
15.404
16.670
14.824
15.376
15.322
15.511
15.281
14.387
14.984
15.047
15.225
15.343
14.527
15.383
15.694
15.289
14.925
15.508
15.625
15.336
15.140
15.123
15.473
15.582
15.634
15.720
14.880
15.179
14.705
15.436
15.678
15.768
15.287
15.288
15.402
14.638
11.427
11.436
11.457
11.408
10.999
11.439
11.344
10.501
11.321
11.467
11.217
11.023
11.123
11.383
10.534
11.227
11.231
11.070
11.113
10.327
10.815
11.112
11.294
11.382
10.448
11.128
10.820
11.244
10.700
11.145
11.416
11.311
11.234
10.951
11.323
11.142
11.435
11.346
10.837
11.031
10.708
11.400
11.448
11.448
11.245
11.297
11.325
10.560
10.566
10.585
10.520
10.557
10.107
10.551
10.454
9.599
10.437
10.589
10.346
10.083
10.215
10.414
9.536
10.344
10.297
10.086
10.302
9.378
9.922
10.240
10.421
10.525
9.633
10.230
9.857
10.336
9.818
10.213
10.604
10.426
10.392
10.029
10.358
10.246
10.457
10.501
9.977
10.140
9.758
10.446
10.513
10.576
10.433
10.419
10.475
9.632
38
SpT
M4.0
M4.5
M4.5
M4.0
M4.5
M4.5
M5.0
M4.0
M4.0
M4.5
M5.0
M4.0
M4.5
M5.5
M4.5
M4.5
M4.0
M4.5
M4.5
M4.0
M4.5
M4.0
M4.0
M4.0
M4.0
M4.5
M5.5
M4.0
M4.5
M4.5
M4.5
M4.0
M4.0
M4.5
M4.5
M4.5
M4.5
M4.5
M4.0
M4.5
M4.0
M4.0
M4.5
M4.5
M4.0
M4.0
M4.0
M4.0
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
d
[pc]
42.3
34.6
35.0
41.9
28.3
34.7
26.6
27.6
40.3
35.1
25.1
35.1
30.0
21.2
22.9
31.5
38.7
29.3
29.8
25.5
26.0
36.6
39.8
41.5
27.0
30.0
16.4
38.9
24.7
30.3
34.3
40.1
38.7
27.7
32.9
30.2
34.6
33.2
32.3
28.7
30.4
41.8
34.8
34.8
38.9
39.9
40.4
28.4
Table A1: (continued).
No.
CMC15
α(J2000)
[deg]
δ(J2000)
[deg]
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
527
528
529
530
531
532
533
534
535
536
537
538
539
540
541
542
543
544
545
546
547
548
549
550
551
552
553
554
555
556
557
558
559
560
561
562
563
564
565
566
567
568
569
570
571
572
573
574
160905.2−080946
160920.6−222205
160931.0−204146
161003.1−272839
161009.5−194720
161014.4−195137
161133.7−202736
161208.1−254758
161212.3+380320
161317.8−371819
161318.8−274402
161320.8−175752
161321.2−175748
161324.5−272613
161335.2+011558
161356.6−245756
161455.1−301453
161500.1−300823
161555.6−124624
161556.6−211218
161658.8−313638
161703.3−214102
161709.4−004842
161721.7−214438
161829.1−303911
161841.8−183239
161852.7−225954
161854.1+263743
161902.1−213809
161926.6−282007
161926.9−122221
161934.4−315005
161947.1−220311
161948.3−221251
161955.0−150616
162027.5−271739
162027.6−210017
162036.4−212312
162118.2−194518
162155.0−215204
162206.5−212709
162229.7−151513
162247.2−323149
162321.6−214644
162329.3+000041
162343.3+164839
162416.4−321213
162555.4−272124
242.271935
242.335972
242.379549
242.512967
242.539611
242.560215
242.890674
243.033905
243.051441
243.324167
243.328723
243.336702
243.338481
243.352393
243.396920
243.485946
243.729760
243.750518
243.981984
243.986147
244.245317
244.264042
244.289380
244.340727
244.621568
244.674523
244.719943
244.725762
244.758920
244.861167
244.862188
244.893720
244.946259
244.951524
244.979365
245.114957
245.115134
245.151668
245.326248
245.479442
245.527408
245.624064
245.697005
245.840185
245.872192
245.930829
246.068419
246.480872
−8.163008
−22.368285
−20.696133
−27.477691
−19.789078
−19.860466
−20.460152
−25.799473
38.055814
−37.305349
−27.734101
−17.964508
−17.963576
−27.437004
1.266125
−24.965814
−30.248194
−30.139935
−12.773342
−21.205124
−31.610678
−21.684039
−0.811933
−21.743989
−30.653130
−18.544436
−22.998349
26.628755
−21.636096
−28.335472
−12.372726
−31.834866
−22.053125
−22.214409
−15.104481
−27.294236
−21.004894
−21.386708
−19.755174
−21.867890
−21.452507
−15.253673
−32.530551
−21.779086
0.011449
16.811098
−32.203637
−27.356751
−111.2
−8.9
−18.5
−11.1
−10.8
−12.6
−15.5
−16.4
−223.4
+1.2
−9.8
+10.7
+5.7
−16.4
+49.0
−15.2
−11.1
−8.5
−171.7
−12.8
−129.8
−22.4
−50.3
−7.5
−9.5
−15.7
−7.1
+94.4
−13.2
−11.2
−1.5
−17.5
−11.0
−16.3
−40.5
−16.7
−12.0
−14.9
−15.8
−15.9
−16.3
−10.1
+3.0
−151.4
−110.3
−81.8
−16.9
−7.4
−34.7
−23.3
−25.7
−23.5
−28.1
−29.4
−23.8
−33.5
+24.8
+10.4
−31.1
−27.2
−19.8
−34.3
+4.4
−21.6
−11.2
−52.2
+0.4
−26.2
−99.0
−23.8
−90.7
−21.8
−24.4
−35.2
−22.1
−32.4
−27.2
−33.4
−20.7
−27.3
−31.2
−28.7
−17.5
−23.3
+3.5
−28.0
−27.6
−18.9
−25.4
−24.0
−21.1
−147.5
−89.7
−59.3
−168.7
−33.1
14.836
15.290
15.861
14.812
15.878
15.251
15.120
15.219
15.224
15.057
14.482
14.964
14.983
14.736
15.340
15.071
14.343
15.695
15.614
15.937
13.394
15.967
14.777
15.375
15.281
15.175
15.265
15.382
15.238
14.719
14.666
15.077
15.766
15.174
14.772
15.288
15.036
15.308
15.167
15.452
15.010
15.270
15.319
15.285
15.215
15.020
13.321
15.060
10.345
10.498
11.129
10.773
11.446
11.214
11.214
11.304
11.104
11.119
10.492
10.816
11.010
10.687
11.294
11.142
10.408
11.477
11.245
11.366
9.329
10.971
10.783
11.209
10.898
11.023
11.101
11.365
11.324
10.774
10.716
11.076
11.491
11.273
10.864
11.164
10.887
10.942
11.213
11.372
11.107
11.361
11.375
10.791
11.139
11.031
9.150
10.857
9.386
9.499
10.138
9.837
10.490
10.234
10.217
10.312
10.211
10.254
9.623
9.871
10.045
9.780
10.362
10.150
9.523
10.574
10.346
10.397
8.475
10.047
9.891
10.259
10.011
10.082
10.103
10.504
10.402
9.876
9.763
10.162
10.545
10.321
10.014
10.234
9.947
10.016
10.333
10.402
10.129
10.430
10.512
9.866
10.249
10.230
8.154
9.975
39
SpT
M5.0
M5.0
M5.0
M4.0
M4.5
M4.0
M4.0
M4.0
M4.5
M4.0
M4.0
M4.5
M4.0
M4.0
M4.0
M4.0
M4.0
M4.5
M4.5
M5.0
M4.0
M5.5
M4.0
M4.5
M4.5
M4.5
M4.5
M4.0
M4.0
M4.0
M4.0
M4.0
M4.5
M4.0
M4.0
M4.5
M4.5
M4.5
M4.0
M4.0
M4.0
M4.0
M4.0
M5.0
M4.0
M4.0
M4.5
M4.5
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
d
[pc]
16.8
18.0
24.1
31.3
34.8
38.4
38.4
40.0
29.7
36.7
27.5
26.0
34.9
30.1
39.8
37.1
26.5
35.3
31.7
26.8
16.1
17.6
31.5
31.2
27.0
28.6
29.7
41.1
40.4
31.3
30.5
36.0
35.5
39.4
32.7
30.6
26.9
27.6
38.3
41.3
36.5
41.1
41.3
20.6
37.1
35.3
12.1
26.5
Table A1: (continued).
No.
CMC15
α(J2000)
[deg]
δ(J2000)
[deg]
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
575
576
577
578
579
580
581
582
583
584
585
586
587
588
589
590
591
592
593
594
595
596
597
598
599
600
601
602
603
604
605
606
607
608
609
610
611
612
613
614
615
616
617
618
619
620
621
622
162627.8−262515
162632.7−262259
162639.9−051409
162853.1−204452
162908.7−253424
162933.7−333219
162956.6−265918
163018.3−312222
163051.3+472643
163105.7−272546
163151.3−271338
163156.6−284612
163411.1−250737
163431.3−061831
163435.1−265803
163458.0−225720
163654.8−145909
163716.3+220012
163721.3+150356
163856.3+243559
163941.6+104958
164009.1−303655
164049.9−261653
164109.9−225444
164153.9−294943
164220.2−293903
164226.9−294116
164410.4+144307
164420.5+011526
164528.9−250247
164603.7−182656
164627.1−182441
164745.2−152642
164929.9−015503
164935.5−001409
164954.7−104444
165003.8−282352
165040.6+304543
165042.7−111757
165351.3+120527
165558.7−062552
165815.5−184500
170042.1−092535
170127.8−202454
170229.5+134101
170324.5−022723
170604.9−213217
170849.0+194309
246.616093
246.636497
246.666408
247.221606
247.286426
247.390517
247.485960
247.576633
247.714060
247.774135
247.964149
247.986146
248.546478
248.630503
248.646389
248.741873
249.228560
249.318263
249.339075
249.734806
249.923402
250.038295
250.208039
250.291400
250.474606
250.584535
250.612410
251.043737
251.085717
251.370667
251.515685
251.613305
251.938548
252.374660
252.398026
252.478036
252.516220
252.669252
252.678155
253.463908
253.994709
254.564603
255.175695
255.366243
255.622935
255.852280
256.520560
257.204406
−26.420926
−26.383066
−5.235908
−20.747966
−25.573338
−33.538642
−26.988487
−31.372788
47.445484
−27.429512
−27.227434
−28.770246
−25.127127
−6.308740
−26.967563
−22.955792
−14.986014
22.003529
15.065723
24.599775
10.832959
−30.615532
−26.281566
−22.912362
−29.828622
−29.650851
−29.687814
14.718695
1.257428
−25.046570
−18.449126
−18.411552
−15.445246
−1.917569
−0.236093
−10.745772
−28.397889
30.762017
−11.299438
12.090911
−6.431138
−18.750225
−9.426627
−20.415168
13.683805
−2.456636
−21.538272
19.719354
−14.6
−18.6
−47.9
−18.2
−18.7
−31.0
−19.4
−36.7
−56.4
−9.3
−19.6
−11.9
−3.6
+56.7
−10.0
−17.2
−1.6
+298.1
−39.8
+116.1
+4.8
−7.2
+3.5
+207.6
−22.8
−6.5
−6.1
−48.7
−25.3
−7.4
−7.9
−115.9
−11.8
−68.4
−9.9
+95.0
−7.9
+98.8
+26.3
−3.8
+44.7
−3.3
−235.0
−21.0
+0.3
−41.1
+160.0
−62.2
−25.2
−27.0
+0.0
−22.9
−29.8
−43.4
−25.1
+12.7
+7.2
−24.2
−32.2
−21.6
−24.9
−16.1
−19.7
−31.9
−25.5
−49.6
+52.8
+44.5
−19.6
−34.1
−34.0
−793.2
−36.4
−31.4
−26.6
−54.2
+34.6
−26.7
−34.1
−85.8
−14.9
−32.4
−39.4
−91.2
−32.8
−75.2
−268.7
−4.9
+42.3
−24.9
−220.0
−24.1
+88.7
+15.0
+167.8
+48.7
14.932
16.685
15.493
14.545
15.123
15.807
15.512
15.937
14.898
15.597
15.372
15.497
16.111
14.857
16.053
15.456
15.132
15.157
15.420
15.426
14.481
15.150
16.694
15.182
15.412
15.450
15.448
15.474
15.506
15.383
15.988
15.445
15.748
15.311
15.175
14.863
15.229
15.919
15.244
16.187
15.530
16.020
14.899
15.209
16.108
15.324
15.798
15.013
10.841
11.452
11.440
10.572
11.021
11.415
11.393
11.449
10.944
11.461
11.396
11.430
10.878
10.935
11.467
11.296
10.771
11.237
11.376
11.348
10.475
11.248
11.282
11.157
11.447
11.493
11.207
11.235
11.374
11.214
11.188
11.407
11.079
11.258
11.182
10.945
11.258
11.331
11.333
11.155
11.375
11.425
10.793
11.012
11.398
11.332
11.421
11.043
9.845
10.490
10.573
9.576
10.132
10.537
10.437
10.573
10.078
10.527
10.525
10.495
9.968
10.100
10.477
10.349
9.840
10.395
10.477
10.474
9.608
10.382
10.386
10.317
10.605
10.675
10.332
10.379
10.529
10.274
10.218
10.529
10.119
10.396
10.334
10.035
10.389
10.434
10.464
10.329
10.549
10.543
9.871
10.175
10.493
10.496
10.531
10.186
40
SpT
M4.0
M5.5
M4.0
M4.0
M4.0
M4.5
M4.5
M5.0
M4.0
M4.5
M4.0
M4.0
M5.5
M4.0
M5.0
M4.5
M4.5
M4.0
M4.0
M4.0
M4.0
M4.0
M6.0
M4.0
M4.0
M4.0
M4.5
M4.5
M4.5
M4.5
M5.0
M4.0
M5.0
M4.0
M4.0
M4.0
M4.0
M5.0
M4.0
M5.5
M4.5
M5.0
M4.0
M4.5
M5.0
M4.0
M4.5
M4.0
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
d
[pc]
32.3
21.9
42.6
28.5
35.1
34.3
33.9
27.9
33.9
35.0
41.7
42.4
16.8
33.7
28.1
32.5
25.5
38.8
41.3
40.8
27.3
39.0
15.6
37.4
42.7
43.6
31.2
31.6
33.7
31.3
24.7
41.9
23.5
39.1
37.8
33.9
39.1
26.4
40.5
19.1
33.7
27.6
31.6
28.5
27.2
40.5
34.4
35.5
Table A1: (continued).
No.
CMC15
α(J2000)
[deg]
δ(J2000)
[deg]
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
623
624
625
626
627
628
629
630
631
632
633
634
635
636
637
638
639
640
641
642
643
644
645
646
647
648
649
650
651
652
653
654
655
656
657
658
659
660
661
662
663
664
665
666
667
668
669
670
171458.7−020850
171616.8−091200
171640.4−130335
172130.7−150617
172251.3−153539
172330.3+371601
172537.6+204725
172904.2+412225
172932.7+093107
172951.3+093337
173103.7+142913
173107.2−023918
173645.4+050856
173803.7+125321
174105.6+301355
174148.8+150156
174225.8−001135
174225.8−001137
174250.3−071102
174549.1+100449
174814.3+133747
174919.2+475605
175156.2+014220
180113.4+094837
180309.1+195907
180422.4+094840
181024.2+412545
181037.0+075609
181636.3+063857
182001.9+162556
182856.2+345639
182917.5+240842
183001.3−372648
183013.1−323822
183547.5+202939
183801.5+341806
184032.4−401058
184150.9−294130
184245.2+255129
184249.7−321247
184251.4−360729
184610.8+333305
184813.1−371248
185409.2−262139
185523.2−240031
185933.3+341614
185955.9+432359
190047.2−364747
258.744923
259.070123
259.168475
260.378009
260.713928
260.876373
261.406939
262.267892
262.386382
262.464150
262.765665
262.780220
264.189527
264.515617
265.273663
265.453440
265.607592
265.607865
265.709930
266.454798
267.059614
267.330218
267.984409
270.306047
270.788256
271.093732
272.600882
272.654525
274.151450
275.008117
277.234514
277.323172
277.505499
277.554870
278.948249
279.506315
280.135392
280.462222
280.688375
280.707251
280.714227
281.545105
282.054735
283.538435
283.847062
284.889044
284.982935
285.197076
−2.147431
−9.200109
−13.059816
−15.104926
−15.594433
37.267099
20.790309
41.373791
9.518868
9.560368
14.486983
−2.655036
5.149159
12.889334
30.232106
15.032379
−0.193104
−0.193611
−7.183927
10.080409
13.629873
47.934815
1.705564
9.810524
19.985379
9.811386
41.429216
7.936084
6.649169
16.432288
34.944307
24.145190
−37.446867
−32.639491
20.494421
34.301712
−40.182925
−29.691846
25.858293
−32.213058
−36.124927
33.551627
−37.213552
−26.361054
−24.008813
34.270817
43.399788
−36.796430
−79.4
−33.7
−79.6
−14.8
−4.6
−139.1
−20.1
−116.9
−22.9
−23.1
−3.3
−48.1
−6.1
+18.3
−42.8
+54.1
+110.0
+110.0
+39.9
+99.0
−63.5
−408.7
−9.1
−13.4
−11.2
+36.8
−105.8
−94.1
+16.4
−125.8
−20.9
+15.2
−10.2
+55.5
+47.1
+59.5
−111.8
+12.4
−10.4
−673.3
−2.3
+88.2
+17.7
+3.9
+42.8
−1.5
+351.4
−12.9
+128.2
−5.4
−103.1
−42.8
−25.2
+38.0
+88.9
−31.1
−40.9
−41.1
+42.2
−17.2
−27.9
+76.9
+74.7
−373.3
−197.6
−197.6
−23.2
+3.1
−85.3
+86.5
−1.5
−39.5
+83.9
+21.9
+53.7
−45.2
−11.7
−48.6
−9.8
+89.3
−42.9
−34.6
−36.5
+72.3
−167.1
−61.7
−16.3
−498.6
−15.5
+79.3
−17.2
−52.0
−44.5
−5.6
+396.6
−12.8
15.448
15.204
14.956
15.191
14.753
15.444
15.623
15.757
15.065
14.352
15.604
14.323
15.481
14.791
15.175
15.096
15.720
15.367
15.467
15.458
14.779
16.438
15.168
14.286
14.604
15.491
15.064
14.980
15.673
16.381
14.743
14.777
15.407
15.680
15.851
16.561
15.028
14.537
15.470
13.451
15.188
15.079
14.987
15.690
15.797
14.727
14.749
15.901
11.478
11.274
10.958
11.263
10.685
11.498
11.362
11.166
10.937
10.414
11.266
10.315
11.210
10.756
11.243
10.873
11.410
11.410
11.304
11.484
10.334
11.214
10.997
10.294
10.655
11.263
11.132
11.012
11.069
11.450
10.665
10.858
11.344
11.443
11.489
11.419
11.028
10.620
11.389
9.544
11.255
10.989
11.049
11.441
11.312
10.700
10.727
11.373
10.623
10.414
10.030
10.424
9.821
10.643
10.474
10.304
10.096
9.471
10.396
9.420
10.368
9.858
10.360
10.028
10.486
10.486
10.451
10.624
9.458
10.285
10.164
9.369
9.758
10.369
10.185
10.127
10.216
10.531
9.792
9.981
10.455
10.596
10.649
10.526
10.154
9.718
10.536
8.679
10.394
10.104
10.197
10.628
10.440
9.848
9.831
10.391
41
SpT
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.5
M5.0
M4.5
M4.0
M4.5
M4.0
M4.5
M4.0
M4.0
M4.5
M4.5
M4.0
M4.5
M4.0
M4.5
M5.5
M4.5
M4.0
M4.0
M4.5
M4.0
M4.0
M5.0
M5.5
M4.0
M4.0
M4.0
M4.5
M4.5
M5.5
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.5
M5.0
M4.0
M4.0
M5.0
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
d
[pc]
43.3
39.4
34.1
39.2
30.1
43.7
33.5
24.5
27.5
26.5
32.0
25.4
31.2
31.1
38.9
26.7
34.2
42.0
32.6
43.4
20.8
19.7
28.3
25.1
29.7
32.0
36.9
35.0
23.4
21.9
29.8
32.6
40.7
34.7
35.5
21.6
35.2
29.2
41.6
17.8
39.1
34.6
35.6
34.7
26.2
30.3
30.7
26.9
Table A1: (continued).
No.
CMC15
α(J2000)
[deg]
δ(J2000)
[deg]
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
671
672
673
674
675
676
677
678
679
680
681
682
683
684
685
686
687
688
689
690
691
692
693
694
695
696
697
698
699
700
701
702
703
704
705
706
707
708
709
710
711
712
713
714
715
716
717
718
190105.0+305716
190206.3−242119
190259.2−202239
190307.6−193955
190333.0−384706
190543.4−271125
190715.9−283429
190937.6+392326
191045.5−131804
191202.7−193637
191226.5−182812
191500.8−284758
192004.7−371654
192118.6−323844
192250.4−241114
192325.1+393434
192621.8+481457
192656.5−252502
192820.8−362010
193358.2−073312
193620.0+354736
193759.6−152647
194122.7−240243
194126.5−113740
194221.2−062024
194347.0−193956
194515.3−060222
194550.8−081504
194913.7+055306
194934.4−130430
195157.6−282503
195311.7+375728
195341.0−061310
195546.6−021237
200311.7−064214
200635.8−153307
200740.7−024047
200822.6−011432
200837.8−254526
201019.1−371855
201104.5+215210
201225.1−244905
201243.6+441357
201458.7−345505
201822.7+000507
202120.3+413920
202152.4−363521
202328.2+082802
285.270972
285.526303
285.746880
285.782056
285.887527
286.431140
286.816334
287.407046
287.689898
288.011481
288.110573
288.753354
290.019934
290.327755
290.710014
290.854954
291.591110
291.735518
292.086736
293.492693
294.083602
294.498708
295.344947
295.360499
295.588367
295.946058
296.313978
296.461806
297.307281
297.393589
297.990358
298.298829
298.420913
298.944428
300.798789
301.649323
301.919855
302.094302
302.157790
302.579981
302.768789
303.104853
303.181980
303.744625
304.594990
305.334857
305.468695
305.867861
30.954685
−24.355290
−20.377616
−19.665414
−38.785267
−27.190543
−28.574824
39.390634
−13.301131
−19.610335
−18.470018
−28.799677
−37.281674
−32.645606
−24.187495
39.576179
48.249355
−25.417395
−36.336289
−7.553596
35.793454
−15.446564
−24.045479
−11.627786
−6.340185
−19.665692
−6.039535
−8.251310
5.885146
−13.075168
−28.417684
37.957816
−6.219453
−2.210546
−6.703891
−15.552096
−2.679813
−1.242479
−25.757264
−37.315313
21.869689
−24.818229
44.232554
−34.918201
0.085508
41.655727
−36.589303
8.467379
−6.5
+37.7
−96.5
−14.2
+39.8
+15.0
+4.3
+6.2
+49.3
+18.9
+73.7
+13.6
+28.2
+153.3
+23.8
+16.3
−125.8
−50.5
+2.5
+38.9
+156.5
+62.9
+43.9
+109.8
+59.8
−120.8
+159.1
+4.1
+116.8
+54.6
+3.3
−7.2
+173.8
−193.4
+36.0
−142.1
+11.1
+21.7
+37.3
+26.8
−65.0
−9.0
+39.8
−138.1
+61.5
−3.0
+63.2
+105.4
−12.1
−75.9
+43.4
−62.4
−110.5
−47.6
−33.8
+129.7
−93.1
−43.5
−85.0
−54.3
+21.3
−47.4
−212.0
−51.7
−39.1
+5.8
−15.8
−24.6
+89.5
−16.6
−36.1
−52.1
−162.1
−132.7
−66.3
−21.2
−2.1
−25.9
−116.8
−2.1
+40.6
+15.1
+1.8
−71.1
−27.5
+19.8
−56.0
−102.9
+10.3
+33.1
+39.4
+49.5
−114.0
−3.9
−44.9
−4.1
13.062
15.703
13.687
14.982
14.793
16.291
15.392
15.351
14.601
15.494
15.455
15.367
15.616
14.744
14.966
14.959
15.502
15.610
15.974
15.267
14.488
15.381
15.382
15.446
14.890
14.783
15.074
15.716
14.555
14.600
15.405
13.780
15.464
15.117
14.682
15.225
15.518
15.614
15.226
15.583
15.580
15.197
15.400
14.386
16.370
14.515
14.895
15.537
9.023
11.335
9.738
11.048
10.674
11.152
11.370
11.328
10.614
11.415
11.317
10.856
11.446
10.506
10.875
10.834
11.427
11.400
11.169
11.261
10.427
11.125
11.449
11.414
10.575
10.761
11.144
11.225
10.651
10.620
11.484
9.116
11.485
11.131
10.745
10.635
11.289
11.347
10.899
11.488
11.181
11.163
11.404
10.325
11.387
10.597
10.956
11.492
8.041
10.448
8.889
10.097
9.727
10.259
10.492
10.433
9.794
10.505
10.455
9.961
10.543
9.638
10.027
10.006
10.597
10.532
10.290
10.391
9.523
10.229
10.593
10.558
9.706
9.861
10.283
10.237
9.799
9.761
10.652
8.224
10.678
10.142
9.909
9.738
10.306
10.438
10.066
10.674
10.278
10.321
10.539
9.472
10.447
9.620
10.017
10.685
42
SpT
M4.0
M4.5
M4.0
M4.0
M4.5
M5.5
M4.0
M4.0
M4.0
M4.0
M4.5
M5.0
M4.5
M4.5
M4.0
M4.5
M4.0
M4.5
M5.0
M4.0
M4.0
M4.5
M4.0
M4.0
M4.5
M4.0
M4.0
M5.0
M4.0
M4.0
M4.0
M5.0
M4.0
M4.0
M4.0
M5.0
M4.5
M4.5
M4.5
M4.0
M4.5
M4.0
M4.0
M4.0
M5.5
M4.0
M4.0
M4.0
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
d
[pc]
14.0
33.1
19.4
35.5
24.4
19.1
41.2
40.4
29.1
42.1
32.8
21.2
34.8
22.6
32.8
26.2
42.3
34.1
24.5
39.2
26.7
30.0
42.7
42.1
23.3
31.1
37.1
25.1
29.6
29.2
43.4
9.5
43.5
36.9
30.9
19.2
32.4
33.2
27.0
43.5
30.8
37.5
41.9
25.5
21.3
28.9
34.1
43.6
Table A1: (continued).
No.
CMC15
α(J2000)
[deg]
δ(J2000)
[deg]
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
719
720
721
722
723
724
725
726
727
728
729
730
731
732
733
734
735
736
737
738
739
740
741
742
743
744
745
746
747
748
749
750
751
752
753
754
755
756
757
758
759
760
761
762
763
764
765
766
202331.9+392033
202334.1+114217
202433.7+410126
202527.1−194803
202753.8+484510
202839.9+275521
202840.2−175035
202856.4−042040
203015.8+352821
203034.8+411532
203039.1+380823
203114.3+260450
203128.2+403256
203129.7+411751
203131.2+410111
203135.5−280517
203142.1+404755
203211.4+403220
203213.8+410052
203237.6+401249
203240.3+415049
203242.8+404135
203244.8+405411
203259.1+404755
203301.0+405242
203303.8+404519
203306.2+404710
203311.2+143017
203336.6+403318
203339.7+405714
203409.1+411524
203441.1+412934
203454.8+412521
203506.0+021816
203508.6+404801
203521.7+415143
203532.7−312952
203558.6+275202
203756.5+394010
203907.1+245747
203941.2−113603
203948.2+414706
204002.4+405516
204005.1−235504
204407.5−011551
204643.8+244205
204727.9+014257
204906.4−263927
305.883222
305.892088
306.140646
306.363195
306.974506
307.166523
307.167815
307.235401
307.566186
307.645002
307.663318
307.809681
307.867878
307.873923
307.880164
307.897955
307.925684
308.047916
308.057719
308.156876
308.168027
308.178596
308.186714
308.246574
308.254282
308.265975
308.276169
308.296828
308.402540
308.415590
308.538212
308.671475
308.728596
308.775340
308.786205
308.840721
308.886341
308.994222
309.485580
309.779952
309.921965
309.951011
310.010348
310.021489
311.031551
311.682610
311.866516
312.276893
39.342652
11.704907
41.024166
−19.800965
48.752963
27.922651
−17.843065
−4.344714
35.472511
41.259104
38.139734
26.080719
40.549035
41.297549
41.019948
−28.088123
40.798716
40.539025
41.014604
40.213662
41.847005
40.693239
40.903275
40.798644
40.878369
40.755500
40.786383
14.504965
40.555170
40.954091
41.256907
41.492859
41.422545
2.304620
40.800292
41.862000
−31.497809
27.867318
39.669627
24.963154
−11.601030
41.785226
40.921162
−23.918004
−1.264271
24.701622
1.716071
−26.657542
−26.7
+45.5
−4.0
+42.2
+236.2
−4.5
−14.3
+193.4
−3.9
−0.3
−1.7
−86.6
−3.4
+0.2
+0.4
+61.4
+109.8
−3.1
−1.1
−3.7
−2.5
+0.3
−2.0
−2.5
−4.9
−4.0
−0.6
−12.7
−0.1
−0.2
−1.0
−2.8
−1.5
−99.3
−0.7
+1.8
−1.9
+35.5
−1.2
+6.7
+101.5
−7.3
−0.5
+9.8
+137.6
+84.6
+109.8
−22.3
+26.6
−139.6
−6.3
−28.9
−5.0
−15.9
−16.7
+74.1
−10.4
−3.9
−3.4
+19.0
−4.0
−4.9
−0.5
−19.3
+55.7
−1.3
−1.3
−4.0
−1.2
−0.7
−3.6
−3.4
−2.6
−0.5
−3.8
−50.3
−5.4
−3.1
−1.6
−1.3
−3.0
−29.8
−7.6
−3.8
−129.7
−20.6
−6.8
−149.4
−145.2
−4.7
−8.3
−121.1
−16.3
−8.3
+17.5
−1.5
15.137
14.984
15.068
14.284
15.026
15.274
14.880
15.366
15.259
14.907
15.070
14.611
14.820
15.411
13.656
14.949
15.332
15.204
15.321
15.212
15.102
14.849
15.417
15.234
14.943
15.001
15.042
15.343
14.726
15.378
15.342
15.294
15.220
14.413
15.431
14.501
15.562
14.871
14.971
15.455
15.520
14.462
14.842
15.242
15.016
15.312
15.295
14.772
11.153
10.937
11.001
10.042
11.037
11.235
10.641
10.955
11.320
10.997
11.135
10.555
10.506
11.384
9.714
10.988
11.303
10.885
11.353
11.231
11.135
10.643
11.487
11.206
10.977
10.971
10.910
11.062
10.614
11.469
11.414
11.084
10.998
10.279
11.424
10.483
11.346
10.510
10.939
11.362
11.392
10.481
10.899
11.247
11.028
10.978
11.321
10.861
10.157
10.135
10.010
9.149
10.189
10.304
9.788
10.090
10.327
10.046
10.155
9.739
9.508
10.402
8.804
10.097
10.448
9.888
10.372
10.290
10.154
9.682
10.495
10.240
10.007
10.082
9.931
10.167
9.632
10.557
10.416
10.099
10.014
9.371
10.452
9.494
10.371
9.633
9.947
10.503
10.505
9.511
9.992
10.402
10.152
10.158
10.423
10.011
43
SpT
M4.0
M4.0
M4.0
M4.5
M4.0
M4.0
M4.5
M4.5
M4.0
M4.0
M4.0
M4.0
M4.5
M4.0
M4.0
M4.0
M4.0
M4.5
M4.0
M4.0
M4.0
M4.5
M4.0
M4.0
M4.0
M4.0
M4.5
M4.5
M4.5
M4.0
M4.0
M4.5
M4.5
M4.5
M4.0
M4.0
M4.5
M4.5
M4.0
M4.0
M4.5
M4.0
M4.0
M4.0
M4.0
M4.5
M4.0
M4.0
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
d
[pc]
37.3
33.8
34.8
18.2
35.4
38.7
24.0
27.7
40.3
34.7
37.0
28.3
22.6
41.5
19.2
34.6
40.0
26.9
40.9
38.7
37.0
24.0
43.5
38.2
34.4
34.3
27.2
29.1
23.7
43.1
42.1
29.4
28.3
20.3
42.3
27.4
33.2
22.6
33.8
41.1
33.9
27.4
33.2
39.0
35.2
28.0
40.3
32.6
Table A1: (continued).
No.
CMC15
α(J2000)
[deg]
δ(J2000)
[deg]
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
767
768
769
770
771
772
773
774
775
776
777
778
779
780
781
782
783
784
785
786
787
788
789
790
791
792
793
794
795
796
797
798
799
800
801
802
803
804
805
806
807
808
809
810
811
812
813
814
204924.9+432746
205023.0+253133
205131.0−154857
205202.7+164359
205431.8+005128
205715.4+284153
210229.9−073544
210702.8+363829
210802.6+481654
210935.4−151858
211047.1+271141
211145.4+371003
211546.2−130246
211637.2+464516
211757.1+460130
211905.3+452530
211929.6+023115
212230.5−333855
212610.2+280856
213249.5−300849
213428.2−184029
213502.8−301347
213739.4+365941
213847.5+050451
213901.7+070034
214219.1+104129
214504.9+020821
214605.6−251538
214746.6+102947
215008.8−043100
215016.9−391743
215140.0+321605
215354.2+032454
215517.3−004623
215534.4−024117
215718.8−352020
220159.8+330506
220214.8+203615
220258.5+124515
220346.7−093841
220559.0+355057
220625.8+213944
220653.3+165500
221213.2−004519
221705.9+294631
221706.0+254128
221828.2+185521
221921.3−161154
312.353832
312.595845
312.879179
313.011305
313.632902
314.314268
315.624843
316.761688
317.011115
317.397531
317.696300
317.939416
318.942767
319.155172
319.488199
319.772269
319.873673
320.627318
321.542517
323.206666
323.617518
323.761805
324.414319
324.698185
324.757475
325.579874
326.270529
326.523558
326.944263
327.536800
327.570586
327.916742
328.475835
328.822430
328.893512
329.328705
330.499438
330.561985
330.744140
330.944646
331.496100
331.607745
331.722368
333.055197
334.274963
334.275358
334.617915
334.839161
43.463022
25.526046
−15.815947
16.733215
0.857888
28.698058
−7.595655
36.641455
48.281938
−15.316224
27.194830
37.167577
−13.046228
46.754465
46.025097
45.425215
2.520866
−33.648629
28.148976
−30.147073
−18.674969
−30.229986
36.994945
5.081033
7.009516
10.691643
2.139190
−25.260571
10.496548
−4.516673
−39.295555
32.268261
3.415273
−0.773139
−2.688312
−35.338911
33.085176
20.604329
12.754296
−9.644760
35.849433
21.662229
16.916819
−0.755306
29.775410
25.691376
18.922523
−16.198513
+26.6
+1.5
+24.5
+0.0
+62.2
+91.2
+78.3
+0.6
−2.2
+119.3
+41.6
−2.1
+31.6
−7.7
+31.8
−119.8
+127.8
+31.9
+80.7
−30.8
+83.1
+26.5
+9.2
+52.8
+74.2
+78.4
+31.2
+84.1
−114.2
+250.1
+128.0
+226.5
+60.4
+64.0
+152.5
+187.1
+64.9
+133.3
+25.4
+155.9
+130.6
+122.8
+104.5
+68.6
+81.2
+23.5
−101.1
−15.6
−52.8
−106.8
−54.4
−33.0
−16.6
−123.4
−126.5
−3.9
+4.7
−198.4
−23.2
−83.9
−60.7
+8.7
−44.8
−67.7
+52.1
−89.4
+5.0
+1.4
−13.9
−0.9
−17.8
−42.9
−51.3
−93.3
−45.9
−136.9
−106.8
−6.1
−56.8
−9.6
−19.8
−52.3
+18.4
−92.4
+58.5
+19.4
−141.8
+4.8
−63.6
+3.4
+3.3
+8.8
+10.9
−18.4
+110.5
−381.2
15.784
15.130
15.403
15.152
14.727
14.820
15.519
15.390
15.220
15.622
15.398
15.034
15.433
16.013
13.698
15.504
15.027
14.758
15.186
14.848
14.990
15.664
15.719
14.684
15.296
15.020
14.937
14.971
15.183
15.255
15.404
14.539
14.985
15.094
15.428
14.571
15.292
15.111
15.310
14.935
15.155
14.710
14.979
14.890
15.368
15.409
15.033
15.258
11.095
11.078
11.219
11.135
10.752
10.542
11.362
11.364
11.299
11.476
11.379
11.017
11.099
11.464
9.673
11.209
10.984
10.455
11.246
10.869
11.041
11.485
11.478
10.721
11.264
10.912
10.991
11.026
11.259
11.130
11.443
10.589
11.067
10.977
11.175
10.631
11.083
11.095
11.396
10.925
11.139
10.769
10.954
10.966
11.421
11.418
10.867
11.254
10.154
10.216
10.338
10.216
9.922
9.685
10.506
10.533
10.305
10.598
10.550
10.162
10.234
10.615
8.807
10.297
10.105
9.566
10.347
9.968
10.156
10.636
10.541
9.872
10.373
10.026
10.139
10.177
10.431
10.277
10.538
9.714
10.165
10.090
10.289
9.800
10.169
10.236
10.544
10.069
10.256
9.943
10.105
10.147
10.532
10.552
10.059
10.349
44
SpT
M5.0
M4.0
M4.5
M4.0
M4.0
M4.5
M4.5
M4.0
M4.0
M4.5
M4.0
M4.0
M4.5
M5.0
M4.0
M4.5
M4.0
M4.5
M4.0
M4.0
M4.0
M4.5
M4.5
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.5
M4.0
M4.0
M4.0
M4.5
M4.5
M4.0
M4.5
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.0
M4.5
M4.0
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
d
[pc]
23.7
36.0
31.3
37.0
31.0
22.9
33.5
41.1
39.9
35.3
41.4
35.0
29.7
28.1
18.9
31.2
34.5
22.0
38.9
32.7
35.4
35.4
35.3
30.6
39.3
33.4
34.6
35.2
39.2
30.1
42.6
28.8
35.9
28.0
30.7
29.3
29.4
36.3
41.7
33.6
37.1
31.3
34.0
34.2
42.2
42.1
26.6
39.1
Table A1: (continued).
No.
CMC15
α(J2000)
[deg]
δ(J2000)
[deg]
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
815
816
817
818
819
820
821
822
823
824
825
826
827
828
829
830
831
832
833
834
835
836
837
838
839
840
841
842
843
844
845
846
847
848
849
222041.6+275504
222831.0+464004
222944.3−182313
223638.2+301130
223913.1+185632
224424.8+001359
225606.4−111706
225810.6−390549
225847.5+185449
230226.0−250842
230341.7+282947
230642.9+132051
230800.6+243704
230837.9+483900
231028.3+431820
231524.9−040910
231732.4+094156
232028.4+394648
232246.0−034344
232330.7−280714
232416.9−152223
232604.1−103725
232904.3+032911
232954.1−122233
232959.4+022834
233129.7+403252
233536.8−060536
233556.4−002332
234109.0−363818
234152.0−025629
234208.6+010918
234622.9+261901
234803.8+225539
234851.3+064307
235325.6−184440
335.173534
337.129306
337.434706
339.159196
339.804738
341.103462
344.026923
344.544418
344.698265
345.608351
345.923978
346.679020
347.002636
347.157937
347.618246
348.853895
349.385347
350.118477
350.691955
350.878318
351.070553
351.517122
352.268309
352.475701
352.497739
352.873892
353.903395
353.985340
355.287893
355.466693
355.536075
356.595582
357.015951
357.214124
358.356691
27.917794
46.667896
−18.387173
30.191794
18.942289
0.233257
−11.285220
−39.097003
18.913614
−25.145031
28.496600
13.347693
24.618004
48.650121
43.305755
−4.152822
9.699145
39.780268
−3.728940
−28.120824
−15.373100
−10.623807
3.486482
−12.375953
2.476162
40.548023
−6.093351
−0.392284
−36.638405
−2.941636
1.155213
26.317213
22.927686
6.718849
−18.744697
+101.2
+61.1
+112.7
+14.3
−42.1
+6.9
+139.8
−46.4
+7.5
−36.8
−25.8
+48.8
−28.0
+106.4
+33.9
−98.0
+141.4
+50.0
+65.0
+109.2
+196.1
+158.3
+78.7
+253.6
−14.6
+54.1
+77.0
+231.4
+85.9
+101.6
+23.7
+34.8
−68.0
−71.8
+106.0
+98.4
−23.4
−61.0
−107.8
−54.4
−102.0
−34.0
−50.2
−86.1
+11.2
+79.2
−99.2
−43.7
−4.7
−8.4
−131.7
+70.0
−3.4
−46.1
−125.2
−51.6
+6.8
−46.0
+140.4
−56.9
−15.2
−35.5
+28.1
−87.9
−74.1
−82.1
−10.9
−81.7
−90.2
−83.2
14.702
15.480
14.782
15.697
15.024
15.343
15.245
14.726
14.855
15.021
15.134
15.528
15.191
14.930
15.599
14.670
15.644
15.499
15.512
15.603
16.144
15.411
15.633
14.682
15.272
15.427
15.166
15.179
15.312
14.665
14.192
15.409
15.033
14.749
16.153
10.707
11.240
10.677
11.457
10.785
11.136
11.324
10.711
10.828
11.021
10.707
11.329
11.265
10.976
11.323
10.602
11.466
11.275
11.317
11.409
11.190
11.145
11.111
10.711
11.360
11.448
11.178
11.062
11.074
10.500
10.194
11.337
10.903
10.529
11.236
9.875
10.375
9.787
10.542
9.929
10.317
10.417
9.812
9.998
10.157
9.823
10.477
10.434
10.128
10.505
9.671
10.658
10.427
10.484
10.506
10.196
10.192
10.188
9.870
10.532
10.636
10.313
10.157
10.219
9.645
9.313
10.492
10.011
9.721
10.384
45
SpT
M4.0
M4.5
M4.0
M4.5
M4.5
M4.5
M4.0
M4.0
M4.0
M4.0
M4.5
M4.5
M4.0
M4.0
M4.5
M4.0
M4.5
M4.5
M4.5
M4.5
M5.5
M4.5
M5.0
M4.0
M4.0
M4.0
M4.0
M4.5
M4.5
M4.5
M4.0
M4.0
M4.5
M4.5
M5.5
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
d
[pc]
30.4
31.6
30.0
35.0
25.7
30.2
40.4
30.4
32.1
35.1
24.8
33.0
39.3
34.4
32.9
28.9
35.1
32.2
32.8
34.2
19.4
30.3
23.9
30.4
41.0
42.7
37.7
29.1
29.3
22.5
24.0
40.6
27.1
22.8
19.9
Table A2: Previously known M-dwarf candidates (in Simbad and/or in Lepine+11).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
000000.3−153448
000022.7+375803
000115.7+065935
000457.6−170937
000530.0−253101
000639.2−070535
000706.4+355642
000853.9+205024
000853.9+282148
000855.2+491856
000959.9−063201
001202.6+020623
001213.4+302844
001319.5+273330
001458.2+021307
001518.8+434434
001715.8−321954
001914.0−145511
001939.3+195104
001943.0+195111
002010.7−054345
002116.5+184355
002158.1+313715
002327.9+241824
002434.9+300229
002602.6+394723
002706.8+494152
002716.4+473103
002801.0+145641
002814.4−322756
002854.8−273333
003253.1−043407
003322.3+144806
003543.1+023313
003544.1−054112
003555.5+102835
003630.2−005441
003800.8+402623
003804.7−325849
003903.4+133016
003933.8+145434
004236.0−161923
004339.4−112608
004420.7+090734
004435.1−185704
004556.7+334711
004641.4+485141
004957.2+070838
+246.3
+253.9
−445.1
+145.6
+272.4
−104.0
−205.0
−266.2
+146.3
+350.2
+252.3
+303.7
+52.7
+16.3
+314.3
+218.1
+201.8
+286.4
+70.3
+69.8
+294.9
+679.6
+291.1
−270.3
+585.9
+226.2
+361.1
+13.5
+165.5
+103.5
+167.7
+73.6
+273.9
+158.0
−3.1
+1088.4
+401.5
−72.3
+247.9
+87.6
+327.9
−143.0
+309.9
+814.8
+279.7
+260.4
−198.5
+160.2
+71.0
−69.0
−85.8
−13.6
−147.0
+87.9
−107.7
−270.2
+48.3
+203.0
+0.5
+64.7
−25.9
−116.4
−110.7
+26.6
−4.5
+18.7
−48.9
−49.8
+35.3
−78.9
+240.1
+127.5
+7.4
+25.5
−230.1
+7.0
−400.6
−50.3
+38.6
−156.6
−72.0
−176.8
−262.4
−388.7
−195.6
+6.2
−186.5
−79.4
+25.0
+247.1
+14.7
−5.8
+184.0
+16.4
−73.7
+3.2
14.565
15.090
15.857
16.015
13.750
14.087
15.587
12.882
15.350
15.727
15.212
14.518
14.216
14.418
15.450
15.201
14.696
15.147
14.927
14.695
15.971
16.127
15.855
13.684
13.984
15.413
13.637
15.115
15.489
14.485
14.701
13.349
15.533
15.432
15.361
14.623
14.995
15.863
15.771
14.869
13.844
14.578
15.567
13.424
15.314
14.704
15.541
15.317
10.474
11.006
11.286
10.997
9.433
9.831
11.476
8.870
11.234
10.864
11.157
10.590
10.242
10.431
11.411
11.218
10.641
10.876
10.926
10.718
11.499
11.320
11.450
9.753
9.776
10.990
9.733
11.103
11.427
10.121
10.759
9.276
11.258
10.517
10.667
10.222
10.996
11.405
10.813
10.937
9.826
10.306
11.234
9.501
11.274
10.183
11.339
11.413
9.627
10.139
10.418
10.084
8.493
8.958
10.598
8.010
10.309
9.980
10.277
9.721
9.410
9.581
10.535
10.396
9.734
9.944
10.078
9.864
10.507
10.420
10.563
8.867
8.892
10.102
8.852
10.253
10.563
9.278
9.899
8.350
10.406
9.543
9.711
9.367
10.136
10.456
9.951
10.064
8.946
9.477
10.343
8.621
10.426
9.314
10.432
10.578
G 273−196
G 171−35
NLTT 58776
2MASS J00045753−1709369
G 266−39
2MASS J00063925−0705354
LP 240−27
GJ 3010
2MASS J00085390+2821484
LP 191−43
LP 644−53
LP 584−75
2MASS J00121341+3028443
2MASS J00131951+2733310
LP 584−88
LP 192−46
2MASS J00171571−3219539
2MASS J00191396−1455113
2MASS J00193931+1951050
2MASS J00194303+1951117
LP 645−4
LHS 1060
LP 292−71
G 131−62
GJ 3033
LP 193−488
LHS 6007
2MASS J00271665+4731006
LP 465−21
2MASS J00281434−3227556
2MASS J00285473−2733337
2MASS J00325313−0434068
LP 465−43
NLTT 1930
LP 645−53
LHS 117
LP 585−58
V* HI And
G 267−143
[SLS2012] PYC J00390+1330
G 32−37B
UCAC3 148−1626
LP 705−93
LHS 1137
LP 766−10
G 132−25
LP 150−44
2MASS J00495723+0708382
46
Table A2: (continued).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
49
50
51
52
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70
71
72
73
74
75
76
77
78
79
80
81
82
83
84
85
86
87
88
89
90
91
92
93
94
95
96
005017.5+083734
005026.9−260713
005448.1+273103
005453.5+174457
005726.0+293234
005801.1+391911
005907.4+410223
005908.2+375239
010013.9+340405
010014.1−073107
010226.8+410143
010630.6−251649
010630.7+301711
010812.2+002756
010918.8−243024
011030.3−112644
011123.5+164830
011125.4+152621
011212.0+054126
011303.6−343819
011513.4+224052
011514.9+414305
011550.2+470202
012210.3+220902
012227.3+192616
012258.4+125203
012315.0+025712
012331.6−234542
012430.7−335502
012619.5+300520
012854.6−264246
012942.6−082358
013029.1−351202
013128.6+250549
013410.5+125752
013638.6+450014
013707.0+421611
013836.9+172618
013921.8−393610
013935.7+162729
014115.9+301610
014340.2−114925
014353.3+001432
014605.1+413049
014751.8+105218
014901.6+251218
015027.1−185137
015105.2−305754
+64.7
+205.2
+340.0
+181.2
+246.2
−102.6
+239.6
+205.6
+226.5
+83.9
−153.8
+366.3
+218.5
−239.3
+277.5
+180.0
+333.0
+181.9
+129.2
+129.9
+275.5
+214.5
+198.6
+237.0
+146.7
+3.1
−340.6
−197.7
+184.5
+259.8
+74.9
+117.6
+250.2
−153.7
−157.1
+15.3
−262.9
+325.1
+120.0
−153.9
+747.2
+57.9
+40.2
+217.5
+212.7
+411.6
−227.2
+102.2
−35.9
+18.0
+7.9
+9.0
+12.1
+34.1
+43.4
+1.0
+4.9
−318.4
−119.7
−208.8
+5.5
−346.9
−186.8
−321.7
−262.3
−129.9
−190.1
−65.6
−418.7
−47.8
−20.1
−152.7
−24.4
−1.9
−372.3
−222.2
−128.8
+43.3
+128.2
−69.6
−306.4
−180.2
−53.7
+34.3
−141.1
+23.0
−237.9
−117.2
−248.1
−182.7
−156.1
−37.1
−25.6
+49.3
+242.3
+302.6
13.801
15.368
14.335
15.450
15.544
13.598
15.473
14.610
15.918
15.269
13.999
15.146
15.613
14.186
13.910
14.781
14.823
13.658
15.317
14.317
14.787
15.201
14.151
12.375
15.722
12.680
16.289
15.453
14.771
15.878
16.226
15.529
15.194
15.764
14.684
15.533
15.546
15.416
13.723
14.831
15.562
15.456
16.522
14.611
15.479
14.913
15.543
14.908
9.745
11.306
10.340
11.148
11.447
9.561
11.377
10.688
11.498
11.256
10.084
11.156
11.225
10.112
9.940
10.703
10.861
9.082
11.320
10.413
10.573
11.094
10.210
8.412
11.492
7.546
11.389
11.166
10.555
11.249
11.462
10.655
11.275
11.423
10.692
11.382
11.415
11.402
9.209
10.800
11.166
11.369
11.169
10.669
11.232
10.672
11.484
10.942
8.897
10.434
9.454
10.267
10.570
8.680
10.508
9.837
10.623
10.385
9.257
10.304
10.353
9.166
9.066
9.804
10.028
8.208
10.485
9.588
9.718
10.210
9.308
7.537
10.589
6.642
10.449
10.312
9.682
10.342
10.557
9.771
10.433
10.620
9.850
10.560
10.506
10.547
8.274
9.967
10.315
10.561
10.258
9.760
10.364
9.773
10.665
10.141
[ZEH2003] RX J0050.2+0837 2
2MASS J00502687−2607132
G 69−32
LP 406−35
LP 294−24
2MASS J00580115+3919111
NLTT 3228
2MASS J00590821+3752399
NLTT 3286
LP 646−49
2MASS J01022695+4101442
LP 826−539
LP 294−50
G 1−47
GJ 2021
G 270−165
G 34−8
GJ 3076
NLTT 3994
GEN\# +6.10050038
LHS 1221
LP 194−43
** FMR 42
G 34−23
2MASS J01222732+1926170
V* U Psc
NLTT 4612
LP 827−167
GJ 2022 C
NLTT 4779
[PS78] 219
2MASS J01294256−0823580
2MASS J01302899−3512002
NLTT 5044
2MASS J01341058+1257530
2MASS J01363862+4500152
NLTT 5383
NLTT 5483
SIPS J0139−3936
LP 408−34
LHS 1280
LP 708−336
2MASS J01435333+0014323
2MASS J01460505+4130493
NLTT 5985
G 94−16
LP 768−566
LP 884−94
47
Table A2: (continued).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
97
98
99
100
101
102
103
104
105
106
107
108
109
110
111
112
113
114
115
116
117
118
119
120
121
122
123
124
125
126
127
128
129
130
131
132
133
134
135
136
137
138
139
140
141
142
143
144
015257.3+083326
015330.7+014755
015349.5+031322
015349.6+442728
015350.7−103214
015407.9−153623
015645.7+303328
015754.7+285701
015845.3+404944
020244.3+133433
020341.8−012847
020501.3+323545
020707.9−181008
020812.2+150842
020904.5+434126
021044.6−093825
021113.6+205822
021135.6−115332
021138.3+080350
021151.6−035403
021159.9+322145
021320.6+364850
021412.6−035744
021621.3−220047
021705.0−300621
021710.1+352631
022022.2−080826
022046.2+025837
022153.3+281114
022206.2+365145
022315.9+291327
022401.4−103904
022408.6−243416
022547.5+243523
022731.3+193525
023139.3+445638
023503.2+410441
023514.9+024753
023644.1+224025
023729.7+002127
023746.1−070550
023917.6−264919
024011.1+422847
024115.2−043218
024127.2−304915
024422.7+105734
024541.3+445702
024820.4+235219
+90.8
+414.8
+344.1
+243.7
+617.3
+90.0
+219.2
+70.8
+396.8
+455.6
+279.8
+285.2
+105.5
+191.1
+180.0
+225.3
+262.1
−123.6
+229.7
−13.8
+520.7
+28.2
+508.2
−115.8
+46.3
+553.6
−202.3
+150.2
+126.9
+409.9
−163.0
−369.2
+159.2
+210.2
+183.4
+94.9
+179.7
+130.5
−42.6
+507.2
+63.8
+29.8
+134.4
+351.6
+89.8
+44.8
+409.9
+186.2
−57.7
+50.3
+34.5
−98.0
−271.8
−289.1
−12.5
−240.5
−70.8
−91.1
+30.0
−88.4
−106.9
−41.9
−31.4
+5.6
−13.4
−160.9
−330.8
−136.4
−231.2
+46.8
−153.6
+243.0
−30.2
−263.0
−213.7
−288.0
−75.4
−142.5
−316.7
−342.4
+56.4
−21.8
−148.9
−52.4
−55.3
−221.2
−374.3
−165.3
−429.4
−213.4
−35.1
−63.4
−25.8
+45.1
−126.3
−25.6
13.496
15.380
14.689
14.756
14.876
13.741
14.449
15.196
15.017
13.669
16.082
14.667
14.659
14.220
15.763
14.555
15.537
15.587
15.547
15.242
15.067
13.490
15.741
16.197
14.670
15.301
14.997
14.070
15.044
16.426
15.338
15.382
15.241
15.701
15.565
13.923
15.369
13.981
14.597
14.463
14.952
13.652
14.934
13.129
15.372
14.724
15.754
14.999
9.238
10.786
10.587
10.416
10.454
9.807
10.323
11.286
10.704
9.652
11.418
10.504
10.698
10.052
10.819
10.649
11.405
11.232
11.312
10.680
10.778
9.367
10.481
11.308
10.578
9.983
10.848
10.064
11.097
11.388
11.068
11.465
10.981
11.384
11.210
9.970
11.373
10.030
10.081
10.547
10.639
9.601
10.991
9.199
11.127
10.301
11.168
10.847
8.358
9.879
9.701
9.547
9.649
8.899
9.449
10.458
9.811
8.802
10.529
9.684
9.749
9.196
9.974
9.806
10.528
10.375
10.389
9.732
9.842
8.518
9.485
10.401
9.717
9.011
10.033
9.202
10.263
10.439
10.158
10.594
10.089
10.545
10.307
9.133
10.522
9.144
9.194
9.689
9.832
8.749
10.150
8.246
10.256
9.452
10.217
9.965
EM* StHA 10
G 159−9
G 159−10
G 133−48
LHS 1311
WT 1243
NLTT 6496
LP 296−59
LP 196−17
GJ 3129
2MASS J02034172−0128474
G 133−63
2MASS J02070786−1810077
NLTT 7084
LP 196−29
LP 709−44
NLTT 7239
LP 709−50
NLTT 7268
2MASS J02115166−0354022
LHS 1352
2MASS J02132062+3648506
LP 649−72
LP 829−41
WISE J021705.03−300621.9
GJ 3147
LP 650−215
GJ 3153
2MASS J02215334+2811145
2MASS J02220614+3651466
G 36−14
LHS 1399
2MASS J02240858−2434163
G 94−65
2MASS J02273126+1935260
2MASS J02313926+4456387
LP 197−24
G 76−8
G 36−26
GJ 3172
LHS 1427
LP 886−73
1RXS J024011.3+422846
G 75−35
WISE J024127.29−304915.1
UCAC3 202−9347
GJ 3179 B
2MASS J02482042+2352191
48
Table A2: (continued).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
145
146
147
148
149
150
151
152
153
154
155
156
157
158
159
160
161
162
163
164
165
166
167
168
169
170
171
172
173
174
175
176
177
178
179
180
181
182
183
184
185
186
187
188
189
190
191
192
025131.1+241314
025151.1+443409
025243.4+332234
025603.9−003633
025613.9+235909
025700.0+464214
025946.4+385535
030133.2+325122
030138.7+322049
030444.1+220321
030615.0+120554
030626.2+171329
030732.1−063649
030746.8+245755
030839.5−384436
030904.6+003112
031002.1−133413
031053.4+005309
031115.4+010630
031130.4+431126
031142.4−153719
031203.9+111851
031323.0+044629
031412.5+284038
031437.2−094017
031718.2−194018
031806.0−202231
031856.7−343317
032105.5−052638
032158.0−163614
032339.1+054115
032436.2+215018
032640.3+051335
032644.9+191439
032730.8+221238
033235.7+284355
033351.3+060842
033410.5+220421
033556.9−103057
033608.7+311838
033631.4−261958
033640.8+032919
033901.6−243406
034033.5−023934
034043.7−145213
034143.8+182406
034231.8+121622
034236.9+221230
+61.1
+168.4
+159.1
+258.3
+75.5
+43.3
+230.8
+337.2
−319.4
+37.8
+226.7
+208.6
+195.9
+228.1
+75.8
−19.5
−57.0
+276.1
+110.3
+7.2
+90.4
+1.5
−173.6
+310.8
−270.7
+519.0
+12.6
+47.7
+69.6
−49.0
+79.8
+127.6
+59.0
−2.7
−39.0
+51.5
+315.4
+312.9
+115.5
+117.6
+85.1
+116.5
+69.5
+105.2
+142.7
+23.9
+203.2
+64.9
−141.8
−111.4
−149.5
+69.6
−168.5
−81.0
−91.4
−117.2
−136.7
−49.3
−2.0
−25.8
−398.0
−126.5
−7.2
−224.6
−292.8
−319.9
−21.5
−232.3
−153.6
−32.7
+458.0
−751.3
−160.5
−216.4
−38.2
−1.6
+21.5
−244.5
−71.7
−42.0
−92.6
−153.8
−53.0
−72.1
+214.7
+106.6
−144.0
−136.3
−26.1
−123.0
−17.2
−44.7
−128.8
−42.2
−24.1
−85.7
15.507
15.601
15.282
14.829
14.200
15.432
14.753
14.820
15.812
14.913
15.661
14.858
14.747
14.260
15.153
15.012
14.966
14.928
15.553
14.456
15.875
15.034
13.273
16.128
15.577
14.967
14.362
14.802
15.177
15.131
13.939
15.309
14.989
14.299
14.055
13.448
15.491
15.606
14.872
13.365
15.619
13.245
14.914
15.604
15.274
14.412
14.189
16.835
11.456
11.307
11.287
10.421
9.977
11.415
10.411
10.829
11.460
10.486
11.288
10.925
10.462
10.132
11.249
10.785
10.990
11.008
10.682
10.526
11.448
10.996
8.775
10.993
11.452
10.980
10.396
10.839
11.031
11.200
9.867
11.290
10.966
10.123
10.044
9.357
11.331
11.355
10.970
9.187
10.675
9.295
10.898
11.470
11.284
10.484
10.157
11.227
10.516
10.426
10.456
9.567
9.072
10.588
9.517
9.944
10.568
9.655
10.425
10.066
9.552
9.267
10.418
9.835
10.082
10.112
9.755
9.624
10.558
10.134
7.833
10.092
10.577
10.169
9.471
9.996
10.219
10.346
9.013
10.398
10.129
9.252
9.194
8.473
10.516
10.475
10.136
8.315
9.763
8.444
9.968
10.616
10.414
9.643
9.275
10.320
2MASS J02513113+2413154
2MASS J02515114+4434093
LP 298−43
LP 591−156
2MASS J02561395+2359105
[SLS2012] PYC J02570+4642
G 134−63
G 37−23
2MASS J03013889+3220498
2MASS J03044407+2203212
LP 471−50
LP 411−54
G 77−24
LP 355−27
WISE J030839.55−384436.3
NLTT 10023
LP 712−11
NLTT 10130
2MASS J03111547+0106307
NLTT 10125
LP 772−14
2MASS J03120387+1118513
V* CD Cet
LHS 1516
WT 1361
LHS 1524
2MASS J03180602−2022297
WISE J031856.73−343317.6
LHS 1536
LP 772−46
PM I03236+0541
LP 356−751
[SLS2012] PYC J03266+0513
GJ 3225
2MASS J03273084+2212382
2MASS J03323578+2843554
NLTT 11229
2MASS J03341053+2204213
LP 713−10
2MASS J03360868+3118398
WISE J033631.50−261958.1
GJ 3237
WISE J033901.64−243406.1
LP 593−39
LP 773−24
2MASS J03414386+1824061
2MASS J03423180+1216225
Cl* Melotte 22 MT 32
49
Table A2: (continued).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
193
194
195
196
197
198
199
200
201
202
203
204
205
206
207
208
209
210
211
212
213
214
215
216
217
218
219
220
221
222
223
224
225
226
227
228
229
230
231
232
233
234
235
236
237
238
239
240
034247.0−242746
034253.2+232649
034322.1−093349
034335.5+262130
034420.8+074154
034659.5+152416
034758.8+232904
035047.0+481235
035059.5+141401
035100.7+141339
035241.7+170103
035336.7+311224
035616.3−391521
035630.4+241718
035646.6+362441
035719.9+410742
035849.1+123022
035915.0+163951
035945.1+215147
040059.5+142045
040253.1+182426
040324.8+082450
040427.0+202430
040620.6+190138
040703.3+201650
040708.1+145956
040730.6−400529
040855.5−312855
040922.2+054626
041233.0+210343
041234.8+352959
041247.3+222326
041305.6+151451
041326.6−013921
041447.3+280305
041534.5+193559
041627.9+205328
041632.0+460635
041643.3+164919
041718.5+084921
041739.7+122453
041818.5+221322
041833.8+182152
041835.9+173057
041903.1+193239
041920.8+043650
041935.4+282721
042039.1+271731
+23.1
+176.7
+400.5
+173.3
−158.7
+222.5
−62.5
+71.0
+65.7
+64.5
+436.7
+143.1
+69.6
+29.6
+128.8
−204.8
+255.3
+141.4
+275.0
+132.0
+133.4
+21.7
+120.3
+107.8
+170.3
+58.7
+282.6
−366.3
+221.9
−0.3
−163.6
+118.4
+126.3
+138.3
+10.6
+215.4
+6.0
−169.0
+101.5
+129.2
+122.7
+91.3
+113.7
+63.3
+124.2
+135.4
+5.9
+4.0
−372.7
−61.2
+302.5
−61.2
+11.6
−25.0
−137.8
−102.5
−74.1
−77.5
−651.6
−72.0
−13.9
−48.0
−84.0
−31.3
−309.1
−27.4
−205.8
−20.9
−36.8
−120.8
−41.8
−26.6
−46.6
−158.0
+35.9
+303.1
−126.1
−23.6
+96.1
−47.8
−21.4
−6.4
−31.6
−46.8
−17.9
−118.2
−23.6
−377.0
−16.5
−8.1
−44.9
−68.9
−44.8
−291.4
−28.8
−31.0
14.893
14.267
14.009
14.716
14.185
14.889
15.792
14.532
14.809
13.405
13.145
14.531
14.824
15.640
14.949
16.174
13.717
15.263
15.152
14.633
14.717
14.773
15.290
15.473
15.617
14.909
15.489
13.831
15.353
14.900
14.977
15.079
15.372
13.298
15.572
14.937
15.228
15.523
15.090
13.225
14.731
16.240
15.591
15.321
14.822
14.335
15.793
14.689
10.929
10.202
9.799
10.772
10.191
10.733
11.347
10.572
10.241
9.436
8.933
10.456
10.460
11.160
10.981
10.903
9.757
11.269
11.092
10.693
10.770
10.647
11.210
11.341
11.450
10.986
11.330
9.775
10.708
10.891
10.642
11.061
11.303
9.375
10.796
10.787
11.054
11.422
11.161
9.030
10.746
11.170
11.490
11.352
10.904
10.427
10.954
10.497
10.042
9.316
8.854
9.903
9.380
9.851
10.492
9.694
9.380
8.579
8.053
9.582
9.602
10.289
10.102
9.949
8.877
10.382
10.243
9.826
9.913
9.775
10.325
10.471
10.556
10.107
10.418
8.823
9.740
9.939
9.790
10.165
10.444
8.504
9.917
9.911
10.085
10.546
10.275
8.182
9.868
10.207
10.601
10.504
10.009
9.565
9.971
9.560
CD−24 1826B
V* LR Tau
LHS 1582
2MASS J03433551+2621311
2MASS J03442081+0741549
LP 473−26
Cl* Melotte 22 MT 88
V* MR Per
2MASS J03505949+1414017
2MASS J03510078+1413398
Wolf 227
LP 301−63
WISE J035616.31−391521.8
V* V692 Tau
LP 248−7
2MASS J03571999+4107426
G 7−14
LP 414−25
LP 357−99
Cl* Melotte 25 REIDA 477
Cl* Melotte 25 REID 42
[SLS2012] PYC J04034+0824
2MASS J04042701+2024303
50
Cl* Melotte 25 REID 64
2MASS J04070817+1459562
2MASS J04073043−4005291
LP 889−37
NLTT 12648
2MASS J04123300+2103433
2MASS J04123491+3529592
Cl* Melotte 25 VA 50
2MASS J04132663−0139211
2MASS J04144739+2803055
LP 414−139
2MASS J04162791+2053285
2MASS J04163215+4606360
Cl* Melotte 25 LH 247
GJ 3270
Cl* Melotte 25 VA 112
2MASS J04181854+2213229
LP 414−158
Cl* Melotte 25 VA 139
G 82−11
V* FR Tau
USNO−B1.0 1172−00072216
Table A2: (continued).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
241
242
243
244
245
246
247
248
249
250
251
252
253
254
255
256
257
258
259
260
261
262
263
264
265
266
267
268
269
270
271
272
273
274
275
276
277
278
279
280
281
282
283
284
285
286
287
288
042109.3+275036
042119.7+120237
042123.4+105202
042135.5+165339
042233.5+390043
042239.8+150344
042254.1+243953
042259.2+255913
042306.1+234602
042312.4+154246
042409.4+150515
042420.2+304433
042421.5+370620
042445.0+270144
042515.5+282927
042519.2+370508
042530.5−095549
042547.0+173240
042604.3+170714
042613.6+465945
042621.7+180000
042632.6−304804
042703.1+240615
042724.1+140707
042745.6−332742
042929.7+261652
043025.3+395057
043052.1−011246
043115.7+104215
043115.7+182006
043123.8+241052
043226.2+182752
043241.0+180923
043331.5−021101
043334.0+204445
043341.7+175040
043348.2+422706
043423.8+205257
043431.2+172220
043437.7+190604
043459.2+173337
043506.1+130804
043513.1+172549
043513.1+225920
043524.6+104452
043528.4+152357
043547.7+252343
043649.1+045110
+1.8
+109.1
+93.4
+138.7
+598.2
+63.7
+5.0
+33.6
+215.7
+110.0
+174.4
−141.3
+47.3
+4.6
+14.6
+402.4
+86.5
+103.3
+111.1
+145.4
+103.8
−64.8
+108.1
+101.2
+47.5
+4.4
+269.8
+129.8
+96.4
+11.4
+4.3
+9.5
+10.4
+229.5
+452.7
+11.0
+210.4
+21.3
+5.9
−195.6
+4.2
+21.0
+12.4
+94.5
+111.8
+96.2
+2.9
+279.8
−28.8
−9.7
−10.4
−42.6
−611.6
−31.7
−22.3
−249.6
−175.1
−29.2
−66.9
−186.1
−57.6
−30.6
−28.8
+5.8
+356.0
−28.9
−36.9
−125.4
−33.1
−472.4
−48.1
−17.0
−1.3
−32.1
−566.8
+33.8
−9.6
−19.9
−20.9
−21.0
−23.6
−261.6
−324.9
−16.8
−201.3
−225.2
−22.5
−66.3
−30.4
−49.3
−25.3
−48.5
−8.3
−31.4
−21.6
−106.6
16.149
15.819
15.020
14.898
14.602
14.968
14.606
13.593
15.383
15.323
14.541
15.404
14.191
15.528
16.775
15.505
16.216
15.348
14.927
15.419
15.226
13.475
15.479
15.352
15.429
15.305
13.132
15.706
14.493
15.466
14.068
15.980
15.659
16.278
13.828
15.720
15.439
15.231
15.344
15.270
15.719
15.029
15.178
15.571
15.492
15.426
14.645
15.840
11.229
11.361
11.049
10.783
10.473
10.917
9.648
9.645
11.135
11.241
10.303
11.451
10.191
11.340
11.258
10.972
11.471
11.189
10.887
11.001
11.119
9.303
11.489
11.401
11.263
10.340
9.113
11.403
10.535
11.210
9.729
11.117
11.311
11.475
9.769
11.274
11.462
11.021
11.205
10.610
10.634
10.953
11.000
11.127
11.179
11.320
10.272
11.254
10.358
10.483
10.190
9.915
9.670
10.062
8.651
8.786
10.233
10.356
9.472
10.617
9.340
10.458
10.328
10.096
10.572
10.316
9.987
10.118
10.253
8.411
10.574
10.529
10.395
9.388
8.246
10.527
9.676
10.304
8.768
10.173
10.341
10.630
8.960
10.313
10.544
10.138
10.234
9.710
9.717
10.102
10.058
10.250
10.282
10.438
9.331
10.418
2MASS J04210934+2750368
Cl* Melotte 25 VA 208
2MASS J04212344+1052021
Cl* Melotte 25 LH 199
LHS 1667
Cl* Melotte 25 HAN 269
2MASS J04225416+2439538
G 8−31
LP 358−167
LP 415−35
V* IO Tau
NLTT 13166
2MASS J04242150+3706208
2MASS J04244506+2701447
2MASS J04251550+2829275
2MASS J04251914+3705083
LP 715−12
Cl* Melotte 25 LH 135
2MASS J04260431+1707145
LP 156−58
SDSS J042621.75+180000.8
LHS 5094
LP 358−268
2MASS J04272407+1407072
WISE J042745.66−332742.6
V* FW Tau
V* V546 Per
2MASS J04305207−0112471
1RXS J043115.6+104217
2MASS J04311578+1820072
V* V927 Tau
2MASS J04322627+1827521
2MASS J04324107+1809239
2MASS J04333153−0211010
GJ 3296
Cl* Melotte 25 LH 48
LP 201−54
LP 415−213
2MASS J04343128+1722201
LP 415−217
Cl* Melotte 25 LH 27
Cl* Melotte 25 LH 3
Cl* Melotte 25 LH 19
V* EZ Tau
51
Cl* Melotte 25 VA 763
2MASS J04354778+2523436
NLTT 13616
Table A2: (continued).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
289
290
291
292
293
294
295
296
297
298
299
300
301
302
303
304
305
306
307
308
309
310
311
312
313
314
315
316
317
318
319
320
321
322
323
324
325
326
327
328
329
330
331
332
333
334
335
336
043702.2+423041
043732.1+164531
043802.4−055614
043809.4+111905
043810.5+154917
043904.5+233319
043905.7+233811
043933.6+413249
043951.6+193934
044033.1−073119
044104.2+255755
044145.6+230158
044159.0−135604
044320.2+294006
044443.7+182429
044505.7+432432
044609.1+064500
044615.2+184629
044617.7−062302
044627.1+173735
044642.6+245903
044712.2+203810
044749.6+124129
044801.0−260301
044857.8+364822
044859.5+153617
045050.3+260728
045051.0+220720
045128.9+103247
045203.8−105822
045229.3+093028
045336.0−283535
045357.0+091558
045435.3+083020
045545.3+301938
045651.4−165530
045703.2+333156
050305.6+212235
050414.7+110324
050505.9+441403
050612.9+043926
050616.7+244610
050647.8+074201
050711.3+143001
050714.4+373042
050827.3−210144
050919.4−134841
051453.6−330429
+162.0
+87.7
−70.5
+85.9
+97.5
−0.9
+8.8
+442.9
+89.3
−32.8
+2.0
−1.5
+285.9
+4.6
+84.0
+372.9
+91.0
+95.2
+263.4
+91.2
+0.9
+83.9
+69.0
+166.1
−1.2
+85.7
+24.8
+631.4
+120.6
−354.3
+164.0
+25.9
+91.8
+135.6
+6.1
+9.4
−78.2
+94.1
−63.2
+92.8
+34.2
−0.6
−174.9
+16.4
−105.5
+36.5
+278.0
+176.7
−204.1
−26.9
−182.6
−9.6
−25.8
−24.6
−23.2
+129.9
−42.0
−315.7
−22.8
−21.8
+30.5
−33.4
−42.2
−633.9
+4.4
−36.7
−220.8
−31.5
−27.3
−95.6
−14.6
+78.3
−368.0
−24.9
−54.7
−433.5
−405.1
−213.2
−351.5
+0.0
−1.4
−191.4
−29.8
−439.2
−336.2
−140.9
+192.6
−29.3
−92.5
−21.1
−205.5
−76.1
−8.0
−15.3
−22.7
+144.6
15.241
14.852
13.834
15.565
15.368
14.852
15.954
15.163
15.627
14.518
15.948
14.718
15.373
15.201
14.513
14.899
14.518
15.234
15.143
15.619
16.175
13.574
15.342
14.990
15.617
15.147
16.657
14.504
15.417
15.464
15.388
14.394
15.345
15.582
15.804
15.275
16.322
14.029
13.139
14.115
12.847
14.822
15.532
15.173
14.713
14.189
15.545
14.310
11.075
10.633
9.730
11.410
11.384
10.479
11.338
11.128
11.365
10.473
10.947
10.738
11.428
10.402
10.561
10.840
10.395
11.087
11.049
11.467
11.261
9.380
11.337
10.773
10.867
11.001
9.152
9.896
11.388
10.502
11.294
10.174
11.308
11.334
11.440
11.330
11.396
9.750
9.144
9.829
8.909
10.792
11.448
10.571
10.284
9.716
10.929
10.089
10.206
9.723
8.818
10.529
10.526
9.617
10.475
10.266
10.441
9.579
9.952
9.854
10.602
9.408
9.655
9.960
9.522
10.188
10.234
10.618
10.338
8.507
10.455
9.936
9.955
10.131
8.305
8.977
10.505
9.606
10.449
9.301
10.445
10.384
10.462
10.502
10.408
8.888
8.311
9.017
8.067
9.815
10.600
9.664
9.397
8.833
10.025
9.171
2MASS J04370219+4230427
52
LP 655−43
2MASS J04390453+2333199
WISE J043905.72+233811.1
2MASS J04393348+4132488
2MASS J04403324−0731177
Haro 6−32
[TLM2010] 2M J044145 B
LP 715−44
Haro 6−36
LP 415−2037
LP 201−108
RX J0446.1+0644
LP 416−26
LP 656−8
LP 416−471
2MASS J04464260+2459034
2MASS J04471225+2038109
LP 476−631
LP 835−18
2MASS J04485783+3648237
LHS 1705
LHS 1706
NLTT 14060
LP 716−10
NLTT 14097
UCAC3 123−12808
NLTT 14154
2MASS J04554535+3019389
LP 776−31
2MASS J04570322+3331584
LP 359−186
GJ 3326
PM I05050+4414
RX J0506.2+0439
2MASS J05061674+2446102
NLTT 14509
[SLS2012] PYC J05071+1430
2MASS J05071449+3730421
2MASS J05082729−2101444
LP 717−3
LTT 2215
Table A2: (continued).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
337
338
339
340
341
342
343
344
345
346
347
348
349
350
351
352
353
354
355
356
357
358
359
360
361
362
363
364
365
366
367
368
369
370
371
372
373
374
375
376
377
378
379
380
381
382
383
384
051517.1+090735
051517.5+233625
051622.7+244522
051836.6−284204
051842.0+303500
051955.0−281749
052349.0+223238
052419.1−160115
052425.7+192206
052623.6+100341
052753.4+312753
052848.2+112054
052944.6−323914
053157.8−030336
053700.7+233044
054025.7+244806
054053.8+085418
054304.6−263538
054307.8+443946
054458.0−245610
055011.7+093949
055246.8+032101
055344.0+315052
055405.1−024822
055543.7+465056
055817.2−043802
055850.2−030832
055853.3+212100
055919.5−091833
060156.4+403206
060229.2+495153
060433.8+412645
060438.8+074154
060524.8−161805
060731.8+471225
061022.4+223419
061156.0+332549
061222.4−080716
061237.8−082622
061955.6+165025
061957.4+202218
062015.3−002339
062051.7+314511
062136.4+322237
062150.4+155413
062351.2+454003
062728.1+212922
063038.6−020550
+79.5
+36.7
+32.7
−38.4
+5.4
+8.9
+226.7
+20.5
−14.2
+32.9
−66.2
−95.9
+150.5
+5.4
+2.4
+1.6
−17.5
+68.5
−119.1
+220.6
+259.4
+174.8
+83.7
+28.7
+8.4
+81.3
+25.1
+55.7
+42.9
−16.8
+58.9
+52.0
+82.4
+328.7
−6.2
+38.7
+129.1
−103.0
−198.7
−19.0
+60.9
−51.4
−71.2
+65.7
+36.3
−28.8
+132.1
−204.4
−306.6
−71.5
−105.3
+435.7
−29.4
+264.4
−305.4
−36.7
−35.2
−217.2
−146.2
−66.4
+100.3
−54.4
−45.6
−400.1
−35.8
+199.5
−108.3
−140.1
+240.1
−78.8
−124.1
−253.9
−534.7
−217.9
−204.5
−444.2
+65.5
−188.2
−855.5
−91.5
−207.5
+134.1
−7.8
−161.0
−407.7
+1.9
−155.3
−103.2
−207.2
−121.9
−432.3
−194.7
+30.5
−285.8
−210.8
−52.0
15.556
14.561
14.991
15.139
15.050
15.498
14.844
13.031
13.769
14.907
15.421
14.178
13.148
13.798
15.942
14.172
14.995
14.606
14.729
14.842
15.159
15.143
14.884
15.142
15.028
15.329
15.584
14.561
14.955
15.491
13.812
15.185
15.049
14.666
13.736
15.598
14.282
16.525
14.971
14.841
14.741
15.359
15.553
15.332
15.420
14.795
15.447
14.731
11.462
10.186
10.651
10.873
10.649
11.356
10.703
8.668
9.464
10.468
11.426
10.174
9.215
9.452
11.435
8.978
10.455
10.568
10.819
10.761
11.186
11.136
10.711
10.723
11.089
11.113
11.404
9.968
10.975
11.238
9.350
11.044
10.636
10.492
9.723
10.644
10.163
11.201
10.861
10.840
10.740
11.307
11.362
11.041
11.389
10.348
11.225
10.729
10.633
9.306
9.746
10.014
9.749
10.530
9.850
7.807
8.564
9.655
10.535
9.331
8.316
8.538
10.543
8.039
9.589
9.717
9.993
9.846
10.333
10.223
9.859
9.806
10.274
10.312
10.591
9.066
10.124
10.384
8.435
10.221
9.784
9.662
8.887
9.746
9.345
10.270
9.961
10.020
9.885
10.434
10.462
10.155
10.553
9.437
10.354
9.857
NLTT 14744
2MASS J05151753+2336260
[SLS2012] PYC J05163+2445
LP 892−32
53
LP 892−36
GJ 1078
2MASS J05241914−1601153
2MASS J05242572+1922070
NLTT 15056
2MASS J05275344+3127540
V* V441 Ori
2MASS J05294468−3239141
PM I05319-0303W
V* V780 Tau
2MASS J05405390+0854183
LP 837−16
2MASS J05430792+4439470
LP 837−20
2MASS J05501174+0939492
2MASS J05524682+0321016
2MASS J05534403+3150526
LP 658−71
** LDS 3680
LP 659−4
LP 659−6
LHS 6097
2MASS J05591958−0918340
2MASS J06015642+4032074
LHS 1809
2MASS J06043383+4126465
2MASS J06043887+0741545
LP 779−17
2MASS J06073185+4712266
NLTT 16144
LHS 6100
2MASS J06122246−0807162
LP 659−20
[SLS2012] PYC J06199+1650
G 104−33
LP 600−8
2MASS J06205178+3145134
2MASS J06213640+3222390
2MASS J06215046+1554140
LP 160−22
2MASS J06272815+2129225
WD 0628−020
Table A2: (continued).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
385
386
387
388
389
390
391
392
393
394
395
396
397
398
399
400
401
402
403
404
405
406
407
408
409
410
411
412
413
414
415
416
417
418
419
420
421
422
423
424
425
426
427
428
429
430
431
432
063038.7−020553
063150.7+412944
063220.2−094329
063529.8−040318
063636.9+061910
063755.4+085859
063756.6−371131
064058.0+494429
064206.9+094640
064334.6+164135
064417.9+412815
064641.0−215016
064707.1+443945
064859.8+382116
065631.0+440154
070006.8−190124
070110.6+155827
070136.5−143717
070155.2+441715
070434.4+165726
070640.4+262459
071111.5+432956
071114.7+102758
071251.0+370733
071442.3−400938
071617.9+330909
072011.3+152354
072217.4+085156
072418.7+382058
072421.1−312557
072851.1−301554
073129.4+024908
073326.7−274904
073505.8+100028
073554.6+333345
073625.1+070442
073847.2+492525
074119.3+123938
074440.1+033308
074540.3+493148
074636.4−253702
075151.3+053257
075154.6−000012
075544.6−274206
075830.4+153000
075852.7+121205
081048.0+010911
081852.9+212703
−77.6
−7.7
−11.1
−287.8
+69.5
−7.6
−47.6
+2.3
−16.0
−215.8
+76.4
−190.4
+102.8
−126.4
+182.3
+155.0
−17.5
−229.4
−106.5
+7.8
−58.9
+350.2
+120.7
+449.3
−20.9
−103.5
−226.9
−160.4
+30.0
−56.0
−221.7
−194.3
−94.4
−252.7
−48.9
−18.4
+43.0
−25.8
−347.3
−101.6
−8.3
−64.2
+248.8
−255.5
−84.0
−0.4
+52.9
−170.8
−213.3
−211.3
−57.0
+180.0
+138.2
−340.3
+116.7
−164.2
−110.4
+39.7
−400.5
−42.8
+47.5
−170.7
−684.6
−74.7
−179.8
+215.8
−167.9
−211.0
−152.6
−572.8
−128.8
−119.1
−10.7
−439.4
−252.3
−62.1
−51.9
+28.8
−274.4
−508.2
−49.2
+208.2
−232.4
−281.1
−496.5
−159.2
−448.8
−174.8
−3.6
−66.1
−742.6
+100.1
−118.4
−13.2
+192.2
+5.2
14.904
14.205
13.781
13.752
16.318
15.105
14.436
15.390
15.556
13.737
15.720
16.364
15.009
14.812
13.889
13.350
15.457
15.664
15.508
14.702
15.120
15.431
15.527
15.121
14.635
13.805
15.422
14.729
14.900
13.732
13.143
16.180
15.290
15.380
15.524
12.555
15.421
15.405
10.563
16.137
12.185
14.034
12.537
15.517
14.428
15.077
14.993
14.734
10.729
9.680
9.848
9.272
11.242
11.163
10.326
10.743
11.398
9.776
11.233
11.220
10.846
10.833
9.923
9.029
11.375
11.252
11.285
10.521
10.847
9.979
11.112
11.114
10.453
9.763
11.110
10.603
10.957
9.788
8.896
11.166
11.009
11.178
11.309
8.180
10.632
11.498
6.581
11.404
7.745
9.966
8.496
11.404
10.429
10.650
10.623
10.676
9.857
8.805
8.984
8.307
10.321
10.262
9.509
9.862
10.496
8.888
10.327
10.354
10.036
9.919
9.073
8.091
10.499
10.321
10.362
9.639
9.948
9.126
10.215
10.265
9.596
8.879
10.236
9.753
10.117
8.889
8.062
10.237
10.080
10.326
10.446
7.282
9.701
10.643
5.698
10.472
6.935
9.089
7.661
10.523
9.561
9.839
9.744
9.832
UCAC3 176−39422
GJ 3396
PM I06323-0943
PM I06354-0403
2MASS J06363696+0619102
2MASS J06375540+0858594
1RXS J063756.9−371132
2MASS J06405810+4944304
Cl* NGC 2264 SBL 513
G 110−14
2MASS J06441792+4128179
LP 839−29
2MASS J06470710+4439458
LP 254−29
LHS 1883
PM I07001-1901
2MASS J07011069+1558280
2MASS J07013658−1437185
2MASS J07015525+4417163
2MASS J07043449+1657273
NLTT 17409
2MASS J07111138+4329590
NLTT 17513
2MASS J07125105+3707340
1RXS J071441.9−400939
GJ 1096
2MASS J07201139+1523554
2MASS J07221747+0851566
1RXS J072418.7+382101
2MASS J07242124−3125577
GJ 2060 C
2MASS J07312949+0249084
2MASS J07332681−2749041
2MASS J07350593+1000283
LP 256−34
GJ 3454
LP 162−47
2MASS J07411937+1239390
V* YZ CMi
NLTT 18368
54
LHS 1950
** LDS 6210
2MASS J07554477−2742068
GJ 3469 B
2MASS J07585271+1212058
NLTT 19068
2MASS J08185301+2127034
Table A2: (continued).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
433
434
435
436
437
438
439
440
441
442
443
444
445
446
447
448
449
450
451
452
453
454
455
456
457
458
459
460
461
462
463
464
465
466
467
468
469
470
471
472
473
474
475
476
477
478
479
480
082012.9+092014
082156.8+174856
082426.7+255536
082430.9+390053
082458.9+414725
082924.1−041618
082949.1+264632
082955.6+163902
083046.3−041340
083123.2−102955
083519.8+140833
083606.3+170046
083720.4−281958
084012.1−364157
084127.2+023726
084908.5+393625
085117.5+460602
085147.1+331519
085240.8+281858
085559.5+065203
085619.5+123948
085929.2+291818
090023.4+215004
090320.9+054014
090440.2−121914
090543.3−084159
090729.2+330443
090848.5+465552
090848.8+115141
090907.9+224741
090950.2−141401
091000.6+090138
091339.9+185913
091402.1+482041
091536.2−103548
091650.7+244855
091752.2+211718
091759.4−182329
091841.3+264551
091918.8+383116
091918.9+383123
092148.9+433027
092246.4−154725
092418.0−400513
092439.6+034623
092645.0+085741
092855.6−072214
092903.6−242904
−158.0
−444.1
−196.4
−233.1
+244.4
+93.1
−201.1
+115.7
+44.7
−592.9
−132.3
+60.9
+149.4
−188.4
−264.5
−382.2
−356.4
−72.7
−491.6
−188.7
−44.8
−6.1
−53.8
−50.2
+91.0
+283.9
−704.1
+103.1
−453.3
−81.2
−130.2
−353.2
−162.8
−115.7
−396.2
−70.9
−70.9
−38.9
−194.4
−244.8
−194.5
−294.1
+433.6
+140.3
−200.3
+156.4
−150.0
−213.9
−387.4
+163.4
−138.4
−141.1
−5.6
−387.3
−547.9
+95.4
+33.4
−322.1
−79.4
−307.7
−184.4
+45.3
−169.4
−335.5
+21.8
−157.8
−237.3
−97.2
−253.5
−83.0
−337.6
−381.6
−683.8
−180.8
−151.5
−278.0
+191.4
−71.8
+74.7
−38.3
−268.4
−109.9
−186.0
−123.3
−73.5
−211.9
−352.5
−42.7
+452.7
−115.5
−254.4
−204.9
−37.3
−99.4
−712.8
−139.7
14.419
15.073
14.689
15.831
14.700
15.195
14.274
15.305
15.535
14.309
13.335
14.721
14.856
15.107
15.889
15.123
15.704
15.637
12.500
15.350
13.792
15.584
15.203
16.141
14.907
15.107
15.525
15.039
14.651
14.656
15.305
14.790
14.949
15.966
13.107
14.819
15.492
16.171
15.950
13.878
14.074
13.342
15.299
14.489
15.040
14.529
14.398
16.079
10.465
10.902
10.618
11.088
10.753
11.281
8.235
11.229
11.242
10.070
9.163
10.815
10.727
11.154
11.351
10.584
11.363
11.417
8.560
11.358
9.585
10.775
9.436
10.766
10.746
10.828
11.308
11.068
10.739
10.474
11.067
10.597
10.997
11.454
8.605
10.466
11.437
11.423
11.269
9.924
10.048
9.431
10.965
10.464
11.055
10.350
10.370
10.841
9.565
10.037
9.705
10.137
9.876
10.404
7.260
10.404
10.376
9.136
8.282
9.987
9.888
10.320
10.451
9.640
10.496
10.567
7.666
10.453
8.708
9.836
8.437
9.832
9.893
9.961
10.482
10.233
9.899
9.616
10.176
9.765
10.087
10.582
7.733
9.603
10.530
10.509
10.291
9.059
9.150
8.490
10.051
9.602
10.173
9.436
9.537
9.910
LHS 6145
LHS 2002
NLTT 19450
LP 209−2
LP 209−4
LP 665−17
V* DX Cnc
2MASS J08295564+1639016
1RXS J083046.4−041344
LHS 2024
2MASS J08351992+1408333
LP 425−244
2MASS J08372042−2819575
2MASS J08401227−3641577
NLTT 20048
LHS 2052
LP 164−63
2MASS J08514713+3315206
* rho Cnc B
NLTT 20552
G 41−8
LP 312−51
LHS 2090
NLTT 20861
LHS 2098
2MASS J09054323−0841581
LHS 2107
LP 165−26
LHS 5144
2MASS J09090798+2247413
2MASS J09095024−1414013
G 46−23
LP 427−15
2MASS J09140220+4820417
LHS 6167
2MASS J09165078+2448559
SDSS J091752.21+211718.2
LP 787−17
GJ 3549 B
GJ 1122 A
GJ 1122 B
GJ 3554
LHS 2132
2MASS J09241790−4005120
NLTT 21687
2MASS J09264503+0857421
LHS 2146
2MASS J09290378−2429041
55
Table A2: (continued).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
481
482
483
484
485
486
487
488
489
490
491
492
493
494
495
496
497
498
499
500
501
502
503
504
505
506
507
508
509
510
511
512
513
514
515
516
517
518
519
520
521
522
523
524
525
526
527
528
092910.9+255808
093248.2+265943
094102.0+220127
094332.1+444521
094423.9+163641
094454.0−122054
094558.2−325328
094627.6−122859
094747.1+283748
095009.0+305213
095104.5+355808
095135.7+404333
095319.6+073650
095355.1+205647
095506.6+342039
095757.9+114828
095856.4+055759
095900.4−300743
100050.2+315545
100146.9+272438
100242.4+145912
100249.0+482731
100336.4+331912
100516.3+170325
100652.0−124654
100704.1+352656
100800.9−143626
101209.0−312445
101320.8+464725
101453.0+212345
101510.8+284146
101811.9−202820
101813.6−202840
101836.0−114303
102119.0+080426
102128.7+171243
102213.4+264720
102351.9+435333
102502.7−090515
102845.7−283037
103232.9+063007
103425.7+461822
103507.8−073238
103832.5−071054
104144.1−311156
104241.3−241603
104514.7+494129
104551.7−230901
−1046.4
−93.5
+485.4
−76.5
+50.5
−345.3
−299.3
−179.2
+141.4
−192.6
−75.2
−133.7
−206.3
−209.4
−33.9
−434.5
−179.5
−34.7
−535.9
+101.7
+127.2
−330.6
+76.7
−154.3
−107.6
−318.1
−369.3
+273.6
−248.3
−192.4
+364.7
−385.1
−392.2
−344.6
−138.6
−255.4
−287.8
+170.5
−424.9
−65.5
−235.3
−420.4
−113.1
−31.2
+355.1
+244.5
+17.1
−245.1
−268.2
+285.9
−530.2
−85.0
−285.9
+50.8
+155.4
−148.9
−247.9
−38.2
+187.5
−146.8
+18.4
+388.1
−244.3
−159.1
−71.2
−6.6
−423.6
−280.5
−244.8
−273.9
−147.2
−185.6
+2.1
−70.4
−96.1
+623.8
−82.3
−223.9
−149.5
+114.2
+114.0
−251.3
−93.2
+44.2
−266.7
−2.1
−336.9
−11.1
−190.1
−102.2
−316.0
+16.9
−270.1
+136.3
−217.8
−141.5
15.611
14.976
13.631
15.384
15.539
13.074
13.396
16.211
15.254
15.000
14.810
15.592
15.515
13.361
15.308
14.073
14.036
15.820
15.537
15.269
13.561
14.754
15.379
15.358
13.841
16.068
15.102
12.807
15.756
13.752
14.663
14.803
13.244
15.457
14.934
15.512
15.409
14.553
14.903
15.684
15.024
15.754
15.591
9.960
15.512
15.642
15.193
14.456
10.906
10.356
9.627
11.456
11.470
8.496
9.204
11.266
11.164
10.708
10.577
11.326
11.355
9.208
11.359
10.092
9.937
11.466
10.261
11.007
9.649
9.963
11.392
11.130
9.749
11.433
10.603
8.848
10.873
9.725
10.737
10.586
8.999
11.079
10.789
11.230
11.338
10.039
10.985
10.953
10.507
11.265
11.189
5.643
11.041
10.277
11.125
10.044
9.958
9.472
8.813
10.597
10.583
7.601
8.279
10.349
10.216
9.870
9.690
10.462
10.449
8.326
10.470
9.176
9.039
10.600
9.275
10.068
8.803
9.005
10.487
10.256
8.902
10.532
9.666
7.993
9.982
8.881
9.823
9.707
8.145
10.223
9.934
10.356
10.510
9.127
10.180
10.026
9.544
10.324
10.358
4.780
10.162
9.338
10.219
9.176
LHS 269
HD 82443B
LHS 2171
2MASS J09433219+4445224
LP 428−32
2MASS J09445422−1220544
2MASS J09455843−3253299
LP 728−23
LP 314−66
2MASS J09500916+3052140
LP 261−75
NLTT 22760
2MASS J09531969+0736501
GJ 3571
LP 261−109
LHS 6179
NLTT 23096
2MASS J09590058−3007441
* 20 LMi B
LP 315−23
G 43−23
LHS 6180
2MASS J10033638+3319126
NLTT 23347
2MASS J10065210−1246543
NLTT 23417
LP 729−33
2MASS J10120908−3124451
LP 167−17
G 54−19
G 118−45
NLTT 23954
NLTT 23956
LP 729−55
NLTT 24099
LP 430−7
LP 316−89
2MASS J10235185+4353332
LHS 2258
2MASS J10284580−2830374
NLTT 24622
GJ 3611 B
LP 670−16
HD 92200
LP 904−51
NLTT 25128
NLTT 25223
LP 849−6
56
Table A2: (continued).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
529
530
531
532
533
534
535
536
537
538
539
540
541
542
543
544
545
546
547
548
549
550
551
552
553
554
555
556
557
558
559
560
561
562
563
564
565
566
567
568
569
570
571
572
573
574
575
576
104712.4+402643
104900.5+474553
105032.6−132612
105214.2+055509
105310.4+415538
105646.2+324627
105703.7+221719
105746.5+045332
105827.9−104630
105906.1+301511
110007.4+211450
110032.8+064131
110035.4+372849
110050.4+120410
110229.3+283400
110354.0+241747
110425.3−174809
110506.8−221254
110533.4+321352
110750.2−342103
110849.3+395512
110953.2−241459
111128.1−265503
111212.4+251957
111238.6+033845
111556.7+184159
111859.5−351140
111930.6+464141
111948.0−163237
112212.0−113216
112242.8+375548
112307.8+255336
112404.3+380810
112453.2+132253
112500.4+431938
112528.6−190154
112931.7+094113
113123.9+053028
113218.2−301951
113223.0+181622
113241.1−265209
113456.6+181707
113931.5−243900
113933.7−304000
114333.0−074549
114742.1+001506
114744.3+004816
114825.9−380927
−294.8
−477.0
−237.1
−699.4
−243.2
−154.5
−158.1
+254.0
−189.5
−531.0
−182.3
−284.1
−716.6
+123.7
−213.4
−533.4
+363.9
−65.4
+125.9
+23.5
−328.2
−11.1
−89.8
+259.5
+240.6
−162.7
−94.8
+304.7
−357.3
−319.0
+245.3
−1009.1
+123.8
−17.1
−524.1
+141.9
−93.4
−321.4
−88.5
−363.9
−101.3
−249.2
−12.8
−88.7
−152.4
−305.9
+605.6
+12.1
−37.5
−183.9
+46.9
−58.3
+7.4
−75.4
−137.3
+183.3
−76.0
−308.1
−36.0
−44.9
−246.8
−119.5
−19.9
−409.9
−311.2
−352.3
+99.3
−246.8
−159.1
+30.1
−19.0
−36.2
−34.7
−10.7
−162.7
−611.5
+54.1
−19.0
+11.3
−327.5
−13.8
−50.4
−207.5
−168.0
−294.9
+69.3
−29.8
+49.3
−38.6
−429.3
+177.4
−25.9
+38.8
−95.3
−1219.2
+52.4
16.760
15.255
15.029
14.159
15.407
14.782
15.925
15.389
13.792
14.772
15.206
15.078
14.746
15.284
15.294
16.342
15.206
15.169
16.020
14.329
15.272
14.416
15.386
15.446
15.355
15.560
15.164
15.028
15.097
16.243
16.600
14.552
13.836
15.726
14.450
14.729
14.952
15.428
16.074
14.137
14.487
14.681
15.338
14.330
15.053
16.350
10.455
15.749
11.384
11.112
11.086
9.834
11.459
10.653
11.287
11.134
9.512
10.543
11.107
11.123
10.659
10.676
11.191
11.430
10.826
10.703
11.408
10.262
10.747
10.144
10.331
11.335
11.098
11.428
11.146
10.087
10.645
11.475
11.284
10.294
9.928
11.043
10.377
10.673
10.954
11.474
9.641
10.175
9.837
10.533
11.353
9.985
10.899
11.189
6.505
11.124
10.399
10.205
10.215
8.941
10.580
9.817
10.350
10.238
8.640
9.651
10.251
10.248
9.746
9.782
10.333
10.502
9.867
9.820
10.498
9.407
9.842
9.260
9.453
10.523
10.243
10.551
10.225
9.199
9.786
10.587
10.323
9.459
9.089
10.070
9.470
9.789
10.072
10.575
8.765
9.338
9.012
9.703
10.443
9.118
10.065
10.235
5.654
10.180
** LDS 4016
LHS 2313
LP 731−65
GJ 3631
LP 213−82
2MASS J10564633+3246278
LP 373−35
NLTT 25837
LP 731−76
GJ 3635
2MASS J11000752+2114505
[ZEH2003] RX J1100.5+0641 5
LHS 2340
GJ 3636
LP 317−39
LHS 2345
LHS 5186
LP 849−51
LP 263−71
2MASS J11075025−3421003
LP 214−42
2MASS J11095327−2414594
1RXS J111128.1−265501
LP 374−7
NLTT 26626
2MASS J11155672+1841593
2MASS J11185965−3511385
LHS 2395
LP 792−14
2MASS J11221219−1132159
LP 264−45
LHS 302
2MASS J11240434+3808108
2MASSI J1124532+132253
LHS 2403
LP 792−59
NLTT 27533
NLTT 27628
NAME SSS 113218−3019
2MASS J11322300+1816223
V* V549 Hya
G 56−47
LP 851−68
2MASS J11393382−3040002
2MASS J11433308−0745491
GJ 3686 B
V* FI Vir
2MASSW J1148259−380927
57
Table A2: (continued).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
577
578
579
580
581
582
583
584
585
586
587
588
589
590
591
592
593
594
595
596
597
598
599
600
601
602
603
604
605
606
607
608
609
610
611
612
613
614
615
616
617
618
619
620
621
622
623
624
114849.4+185653
115155.3−013132
115206.6+034119
115257.9+242845
115745.5−014902
120027.4−340537
120028.2−000612
120412.5+051412
120446.3+022400
120513.9−253349
120546.6−184934
120617.4+123024
120624.9+001602
120818.2−210106
120843.8−113346
120906.7+473604
120906.8+473534
121028.4−131025
121314.9−210831
121408.6−234516
121416.5+003726
121731.6+251826
121837.8−202407
121841.9−060912
121847.1+294448
121948.7−233205
122004.9−181259
122126.6+303837
122127.0+303835
122203.9−062913
122229.4+400337
122250.5−040446
122501.0+232316
122520.6−174946
122651.3−331612
122657.3+270053
122702.0−254502
122850.5−083424
122945.2−284731
122954.3−052722
123124.1−063801
123317.3+090115
123405.0+134545
123517.2+131806
123548.9−395024
123628.5+351200
123943.5+253045
124016.8+125359
+24.3
+145.4
−1.0
−321.1
+397.7
−54.8
−102.8
−187.9
−203.0
+189.3
−14.6
−182.2
+39.4
+36.5
+245.7
+587.4
+587.1
+242.8
−373.0
+38.8
−956.8
+26.6
−324.6
+106.7
−207.2
−221.6
−241.3
−198.3
−110.9
+52.4
−169.9
−188.9
−136.0
−119.0
−66.2
+88.6
−298.9
−169.5
−99.4
−717.2
+449.2
−1756.9
+58.6
+93.8
−50.4
−351.6
−179.9
−259.8
−304.9
−153.3
+229.9
+77.3
−204.7
−15.4
−80.2
−151.8
−1.0
−215.1
−312.7
+22.8
−127.5
−274.2
−325.6
−297.2
−297.8
−348.4
+128.9
+84.7
−278.4
−69.5
+34.5
−31.5
−413.8
−25.0
+50.2
−262.0
−310.3
−329.0
+8.2
−334.1
−304.4
−14.4
−25.9
−245.2
−256.6
−82.4
−24.0
−408.2
−226.0
+211.8
−156.7
+203.2
−27.0
−117.4
−152.2
−1.1
15.093
14.897
15.317
13.875
15.302
13.767
15.446
14.764
15.797
15.387
15.457
15.031
14.393
15.843
15.710
14.360
15.383
13.202
14.973
13.245
13.035
15.431
14.927
14.135
15.593
14.526
14.858
14.632
14.479
15.180
14.917
13.716
15.694
15.175
15.361
14.343
14.946
15.552
15.741
13.527
15.398
11.804
15.185
17.170
13.737
13.153
14.296
15.749
10.876
10.544
11.397
9.937
10.905
9.606
11.287
10.217
11.401
11.470
11.199
11.127
10.348
11.115
11.000
10.239
11.095
9.292
11.071
9.067
8.456
11.395
10.891
10.117
11.021
10.489
10.564
10.057
10.057
10.987
10.966
9.662
11.456
10.894
10.691
10.197
10.837
11.449
11.129
8.818
11.328
6.995
11.217
11.225
9.790
9.113
10.242
11.460
10.030
9.643
10.526
9.016
10.024
8.723
10.372
9.317
10.567
10.606
10.317
10.240
9.475
10.231
10.175
9.346
10.225
8.412
10.240
8.234
7.540
10.494
10.033
9.280
10.089
9.580
9.623
9.169
9.169
10.118
10.121
8.825
10.619
9.993
9.783
9.320
9.928
10.624
10.269
7.962
10.434
6.042
10.373
10.365
8.943
8.261
9.394
10.554
LP 433−58
LP 613−62
LHS 2466
G 121−28
2MASS J11574552−0149023
2MASS J12002750−3405371
2MASS J12002826−0006123
NLTT 29470
NLTT 29510
LP 852−6
** WNO 54B
2MASS J12061746+1230249
2MASS J12062495+0016025
LP 794−23
LP 734−29
LHS 2516
LHS 2517
LP 734−34
LP 794−38
2MASS J12140866−2345172
GJ 1154
2MASS J12173161+2518272
LP 794−49
2MASS J12184187−0609123
LP 320−359
LP 52−34
LP 794−53
G 148−47
G 148−48
LP 675−4
2MASS J12222948+4003372
G 13−33
LP 376−62
2MASS J12252074−1749468
2MASS J12265135−3316124
V* CX Com
LP 852−50
LP 675−62
LP 909−5
LHS 2567
LHS 5217
Wolf 424
2MASS J12340501+1345458
NLTT 31198
TWA 11C
G 123−45
GJ 3739
LP 495−235
58
Table A2: (continued).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
625
626
627
628
629
630
631
632
633
634
635
636
637
638
639
640
641
642
643
644
645
646
647
648
649
650
651
652
653
654
655
656
657
658
659
660
661
662
663
664
665
666
667
668
669
670
671
672
124128.9+190500
124229.6+250341
124400.6−111030
124422.7+042123
124853.4+120432
125431.9+445934
125450.7+115914
125750.6+375950
125923.9+074354
130033.3+225540
130033.4+054108
130040.1−201045
130425.8+140510
130523.7+211208
130650.3+305052
130710.9+150431
130720.7−101946
130841.1+090658
130934.9+285906
131012.4+474517
131121.5+283240
131151.7+252050
131420.3+132000
131551.1+400608
131634.5−273913
132017.4−022413
132138.0+395948
132154.0−142409
132426.3−105222
132440.8+005932
132657.9+150542
132726.7−334546
132909.8+111837
133002.6−084226
133031.0+190934
133239.0+305906
133328.0+123850
133600.0+402412
133840.9−113208
133915.9+092236
133938.6−205818
134019.0+471228
134341.6−400229
134618.5+071337
134809.1+042916
134813.3+233648
134840.8−051710
134848.6+040601
+68.6
+22.7
−483.7
+32.6
+229.8
−650.2
−267.7
+43.6
−680.4
+51.4
−942.4
−291.1
−245.7
−193.3
+173.8
+59.0
−359.1
−200.6
−348.6
−634.1
−410.9
−454.0
−242.4
+135.1
−125.5
+75.8
−40.5
−218.2
−25.4
−115.0
+58.8
+33.8
−71.3
−1117.6
−506.3
−199.1
−87.5
+35.8
+144.1
+84.3
−142.6
+285.2
+222.6
+107.0
−168.5
−1479.1
+244.8
−3.8
−305.4
+16.2
−155.3
+7.5
−145.5
−267.9
−396.5
+79.1
+2.0
−13.4
+225.4
−153.1
−28.0
+45.5
−475.0
−169.7
−45.5
−128.0
−197.8
−612.4
−448.0
−164.4
−176.1
−85.7
−143.0
−201.0
+41.3
+78.3
−32.2
−439.1
+11.1
−15.5
−190.4
−471.3
−1289.1
−81.2
−344.5
+29.8
−88.7
−314.9
−118.8
−486.2
−108.5
−115.6
−66.9
+118.3
−464.2
−182.5
14.284
14.728
13.582
15.079
15.308
15.332
15.013
15.146
15.324
15.119
12.744
14.822
15.293
15.257
14.802
15.789
15.040
15.379
13.520
13.822
15.287
15.030
15.082
14.608
15.714
14.559
14.614
13.757
15.381
13.879
15.274
17.236
14.376
13.694
14.129
13.687
15.057
14.858
13.664
14.514
15.364
14.767
14.328
14.689
15.089
14.692
14.244
13.690
10.368
10.734
9.516
10.788
11.400
10.874
10.509
10.948
10.740
11.016
8.553
10.814
11.231
11.323
10.226
11.363
10.908
11.267
9.476
9.584
10.841
10.736
9.754
10.696
11.479
10.636
10.608
9.817
11.388
9.976
11.079
9.680
10.452
9.599
10.065
9.620
11.107
10.717
9.714
10.526
11.406
10.685
10.137
10.726
10.746
10.082
10.329
9.755
9.477
9.790
8.674
9.958
10.570
9.986
9.621
10.002
9.838
10.184
7.660
9.918
10.374
10.481
9.315
10.459
10.019
10.326
8.612
8.687
9.966
9.843
8.794
9.841
10.611
9.817
9.767
8.985
10.532
9.091
10.166
8.833
9.485
8.749
9.221
8.762
10.267
9.823
8.814
9.629
10.580
9.864
9.248
9.792
9.839
9.179
9.403
8.882
G 59−34
LP 377−54
LHS 5226
LHS 2619
2MASS J12485345+1204326
LHS 2650
LP 496−48
LHS 2655
LHS 2657
V* KZ Com
Wolf 461
LP 796−24
NLTT 32773
LP 378−405
LHS 2674a
NLTT 32923
LP 736−27
NLTT 33004
GJ 1167 A
LHS 2686
LHS 2691
LHS 5240
NLTT 33370
2MASS J13155111+4006086
LP 910−62
LP 617−34
LP 218−84
LP 737−51
59
LHS 6253
LP 437−81
LHS 5246
NLTT 34250
BD−07 3632B
LHS 355
** LDS 1392
LP 498−6
2MASS J13360002+4024118
UCAC3 157−131101
NLTT 34786
LP 798−75
LHS 2777
2MASS J13434146−4002292
2MASS J13461853+0713382
NLTT 35270
LHS 362
LHS 2804
Wolf 1494
Table A2: (continued).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
673
674
675
676
677
678
679
680
681
682
683
684
685
686
687
688
689
690
691
692
693
694
695
696
697
698
699
700
701
702
703
704
705
706
707
708
709
710
711
712
713
714
715
716
717
718
719
720
135028.0+052736
135035.8+033038
135157.0−175849
135620.4−280350
135816.0−120258
135820.7+110049
140035.3+213301
140133.1+122726
140223.4+430059
140536.9−320840
140555.9−164332
140651.4+313346
140735.4−060051
140931.9+413808
140951.6+072425
141304.7−120127
141320.5+002304
141415.2+284724
141545.7+062505
141702.7+314246
141707.3+085136
141929.5+025436
142036.4+313004
142052.7+365717
142055.4+121806
142219.9+235235
142243.3+162446
142307.7−221710
142323.7−145533
142343.7+142651
142513.1−162455
142524.1+213151
142534.6+254005
142649.7−325649
142756.0−002231
142756.4−002219
142804.1+135613
142831.5+455433
142837.9+405704
142959.5+293401
143104.4−030716
143152.8−151551
143153.5−134611
143208.4+081131
143331.3+341747
143345.6−312441
143404.7−182411
143718.4+265259
−127.2
−804.9
−110.9
−507.8
−335.9
+197.9
−405.6
−453.1
−132.0
+81.0
−185.6
+53.4
−305.9
−219.3
−192.0
−619.7
+76.7
+209.9
+249.0
−582.7
−139.4
−199.6
−207.4
−1353.2
−383.5
−248.8
−188.9
−273.1
−164.0
+331.5
−368.6
−220.3
−51.3
+104.0
+528.3
−276.1
−360.2
−873.5
+216.3
−232.0
−335.0
+153.1
−157.9
−512.2
−98.4
−27.3
−503.7
−225.3
−116.0
−112.0
−17.2
−86.3
+41.2
−483.3
−145.5
−420.9
+92.8
−204.4
−57.5
−375.1
−684.4
+73.3
−49.9
−381.3
−160.4
−287.5
−128.5
−147.4
+17.9
−146.5
−63.5
+226.6
−138.0
+40.6
+39.3
−464.4
+306.9
−548.8
+20.0
+105.8
−15.5
−18.1
−85.6
+251.2
−491.1
+105.2
−177.0
−471.1
+15.8
−86.1
−198.6
+28.1
−36.1
−28.7
+26.4
+87.2
15.451
14.699
14.913
14.444
13.808
15.328
15.172
14.945
15.177
14.669
14.627
15.159
15.154
15.189
15.409
13.248
14.845
15.312
14.663
12.489
13.229
14.328
15.092
15.642
14.882
14.818
14.416
14.303
15.397
16.521
16.485
15.507
16.640
15.339
13.324
13.422
16.647
16.177
15.277
14.014
14.274
15.245
15.323
14.993
16.674
15.304
13.729
15.143
11.237
10.685
10.823
10.480
9.728
10.830
11.074
11.004
11.037
10.701
10.721
10.893
10.880
10.706
11.087
9.040
10.741
10.935
10.681
8.443
9.109
9.954
10.786
11.054
10.912
10.516
10.303
10.402
11.062
11.218
11.477
11.034
11.083
11.181
9.305
9.345
11.014
11.336
11.354
10.072
10.212
11.115
11.247
10.108
11.451
11.310
9.580
11.022
10.339
9.789
9.927
9.565
8.887
9.988
10.270
10.191
10.126
9.800
9.857
10.038
9.973
9.848
10.140
8.163
9.880
10.075
9.771
7.609
8.198
9.072
9.907
10.254
10.036
9.647
9.452
9.504
10.191
10.256
10.488
10.144
10.105
10.292
8.403
8.461
10.026
10.434
10.516
9.238
9.327
10.273
10.375
9.166
10.554
10.422
8.708
10.125
2MASS J13502806+0527368
LHS 2811
LP 798−49
LHS 2826
LP 739−2
LHS 2831
G 150−56
LHS 2844
2MASS J14022347+4300591
LP 912−48
LP 799−63
LP 324−70
LHS 2862
LP 220−50
NLTT 36435
V* GQ Vir
2MASS J14132052+0023047
LP 325−4
NLTT 36747
GJ 3839
PM I14171+0851
NLTT 36959
LP 325−24
LHS 370
2MASS J14205545+1218068
LP 381−49
NLTT 37131
LHS 2906
LP 740−6
LHS 2909
LP 800−58
NLTT 37289
2MASS J14253465+2540050
2MASS J14264969−3256489
GJ 1183 A
I14279-002En
LHS 2919
LHS 2921
LP 221−118
LHS 2925
60
LP 740−58
LP 740−25
LHS 2935
NDWFS J143331.4+341747
2MASS J14334561−3124412
LHS 5273
LP 325−68
Table A2: (continued).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
721
722
723
724
725
726
727
728
729
730
731
732
733
734
735
736
737
738
739
740
741
742
743
744
745
746
747
748
749
750
751
752
753
754
755
756
757
758
759
760
761
762
763
764
765
766
767
768
143723.8−024250
144158.7−164902
144347.0−130715
144414.9−271725
144433.3+364159
144440.0−221447
144600.8+463323
145158.0+025912
145337.1+113412
145410.4−204129
145627.1+175459
145925.0+361832
150049.9−153308
151012.0+462405
151315.8−113333
151411.5+030046
151416.8−095839
151628.0−210216
151640.6+391048
151655.7−003711
151831.4+203628
151907.8+142447
151921.1+340342
152115.9+394516
152332.6+220326
152351.1+172757
152419.6+201125
152543.5+311211
152724.1+371415
152725.4+173132
152745.0−090135
152902.8+464623
152944.0+425247
153030.3+092601
153109.5−350457
153154.1+285109
153340.4−391747
153427.0+152832
153450.8+180012
153507.5−065522
153535.7+291257
154554.4−044823
154623.3+310254
154715.1+014921
154740.6+224116
155009.7−202912
155042.6−035846
155051.4+182538
−360.1
−195.7
−6.3
−264.9
−49.2
−113.6
+481.2
−75.1
+73.8
−105.6
−849.2
−123.9
−385.6
+389.9
−62.9
+149.1
−127.0
−213.0
−209.5
−119.3
+10.1
−81.0
−168.4
−438.4
−21.5
−399.7
−144.2
+20.0
−142.2
+10.7
+25.1
−118.3
+423.7
−185.4
−46.9
−545.7
−47.4
−123.6
−221.5
−9.7
−203.0
−528.6
−320.2
−231.1
−180.9
−190.9
−19.5
−21.2
−28.1
−260.0
+4.7
−42.6
−108.8
−334.4
−399.5
−159.1
−724.6
−277.6
+494.8
+76.1
−134.7
−398.1
−69.0
−72.0
−126.3
−194.5
−60.1
−190.9
+94.8
−29.4
−202.5
+182.0
−283.0
−1261.2
+95.8
−245.8
+121.5
−183.5
−307.5
−21.9
−617.9
+182.8
−32.6
+34.1
−68.5
−191.0
−325.5
−16.2
+167.6
−282.9
+250.3
−53.4
−29.5
−308.0
−26.8
−262.2
15.261
14.271
10.463
14.994
14.680
14.701
14.061
15.234
14.700
14.362
15.134
14.292
15.508
14.542
15.292
15.507
13.589
15.668
16.361
13.884
14.786
15.055
14.669
15.737
15.384
13.116
15.057
15.096
15.073
15.577
14.473
14.075
13.571
14.431
14.669
13.681
13.743
14.866
14.958
14.607
15.269
16.078
15.880
15.932
13.589
14.927
15.313
14.958
11.312
10.225
6.539
10.891
10.727
10.569
10.138
11.277
10.577
10.256
10.742
10.257
11.494
10.629
11.260
11.252
9.665
11.478
10.796
9.960
10.119
11.024
10.460
10.732
11.172
9.105
11.033
10.651
11.043
11.370
10.552
9.942
9.587
9.569
10.718
9.673
9.837
10.773
10.595
10.571
11.126
11.341
11.135
10.637
9.543
10.896
10.447
10.848
10.500
9.390
5.570
10.036
9.871
9.644
9.308
10.440
9.652
9.348
9.852
9.377
10.545
9.810
10.392
10.343
8.780
10.594
9.813
9.105
9.268
10.200
9.537
9.745
10.325
8.279
10.154
9.699
10.239
10.511
9.632
9.114
8.719
8.661
9.797
8.820
9.021
9.950
9.713
9.705
10.249
10.426
10.264
9.667
8.647
9.999
9.470
9.957
LP 620−41
2MASS J14415883−1649008
HD 129603
LP 858−20
2MASS J14443334+3642002
LP 858−23
LHS 2973
2MASS J14515804+0259130
LHS 2995
LP 801−25
LHS 3001
2MASS J14592508+3618321
LP 741−28
LHS 3031
2MASS J15131587−1133329
2MASS J15141149+0300467
PM I15142-0958
LP 802−13
LP 222−65
2MASS J15165576−0037116
2MASS J15183145+2036279
2MASS J15190781+1424478
2MASS J15192126+3403431
NLTT 40017
NLTT 40109
LHS 396
2MASS J15241967+2011252
NLTT 40208
2MASS J15272423+3714148
LP 442−53
GJ 586 C
2MASS J15290296+4646240
LHS 3075
NLTT 40406
2MASS J15310958−3504571
GJ 3910
[SZB2012] 75
LP 443−16
LP 443−17
61
2MASS J15353572+2912577
LHS 3112
LP 328−40
NLTT 41186
2MASS J15474070+2241165
LP 803−37
NLTT 41333
Table A2: (continued).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
769
770
771
772
773
774
775
776
777
778
779
780
781
782
783
784
785
786
787
788
789
790
791
792
793
794
795
796
797
798
799
800
801
802
803
804
805
806
807
808
809
810
811
812
813
814
815
816
155244.6−262315
155531.7+351203
155836.2−234802
155918.3−221043
155929.2+232139
160015.6−223158
160110.3−222227
160113.9−251628
160121.5−223726
160123.7−241948
160127.7+211613
160129.8−224838
160144.4+302741
160158.9−224037
160241.6+013158
160350.0−180545
160413.1+233138
160419.9−061648
160451.5−210417
160501.7−241133
160628.7−200357
160629.3−240723
160633.7+405422
160728.5−240754
160744.4−203603
160758.7−244132
160843.0−190051
160903.9−193945
160959.3−180009
161001.8−234943
161021.5−194132
161026.3−193951
161036.2+094715
161058.3−063134
161116.6−193910
161248.2+110417
161310.2−190413
161411.5−142131
161530.3−325102
161554.8−231514
161620.1−234414
161910.5+195726
162107.4+150431
162141.2−221205
162357.2−262024
162524.0+485416
162619.7+364056
162648.0−172335
+213.7
−231.7
−13.9
−12.7
−329.7
−7.4
−13.8
−13.0
−10.6
−46.3
−62.9
−9.8
−140.8
−20.3
−139.9
−5.3
−160.6
−68.7
−13.4
−8.1
−19.3
−325.9
−719.3
−15.8
−10.0
−5.9
−11.8
−7.8
−11.0
−11.0
−5.0
−10.8
+1.4
−51.1
−14.4
−331.7
−7.7
+116.6
−228.1
−7.2
−13.7
+17.9
−326.7
−14.9
−7.4
−230.5
−194.1
−330.5
−455.5
+156.2
−16.0
−26.3
+513.0
−28.2
−29.7
−15.5
−20.2
−54.8
−89.5
−31.5
+125.7
−26.6
−536.9
−23.8
+12.7
−862.7
−28.0
−18.5
−32.0
+207.6
+160.6
−30.3
−20.9
−23.9
−26.0
−35.1
−26.3
−21.7
−2.8
−29.9
−584.3
−189.2
−25.4
+325.7
−32.1
−168.1
−220.7
−15.8
−29.4
−9.8
+94.4
−29.1
−20.8
+309.5
+852.8
−411.7
15.773
13.034
15.055
15.573
14.918
15.285
15.116
15.370
15.154
16.078
14.675
15.835
14.537
15.375
16.136
16.417
14.373
14.983
15.806
14.980
15.824
14.288
16.135
15.381
14.194
14.909
15.584
15.468
15.630
15.387
14.946
15.813
15.700
16.776
14.483
15.551
14.709
14.727
14.175
15.345
15.434
15.184
15.204
15.191
15.282
14.765
15.720
13.707
10.258
8.928
11.110
11.044
10.975
11.365
10.732
11.357
11.026
11.448
10.772
11.480
10.427
11.350
10.887
11.489
9.971
10.452
11.283
10.845
11.442
10.364
11.050
11.139
10.076
10.752
11.245
11.338
11.306
11.062
10.826
11.314
11.331
11.348
10.525
11.362
10.628
10.128
10.272
11.275
11.079
10.967
11.270
10.909
11.188
10.823
11.430
9.548
9.315
8.041
10.192
10.073
10.066
10.442
9.758
10.419
10.052
10.541
9.832
10.490
9.540
10.434
10.033
10.499
9.065
9.548
10.341
9.914
10.464
9.511
10.072
10.247
9.077
9.828
10.268
10.369
10.343
10.134
9.860
10.402
10.502
10.371
9.547
10.510
9.647
9.234
9.421
10.329
10.187
10.156
10.440
9.941
10.235
9.971
10.535
8.682
LHS 5303
G 180−11A
UCAC3 133−177729
2MASS J15591839−2210430
LHS 3140
2MASS J16001567−2231580
2MASS J16011037−2222276
62
2MASS J16012156−2237265
2MASS J16012373−2419483
[SLS2012] PYC J16014+2116
2MASS J16012985−2248386
GJ 3936 B
2MASS J16015894−2240368
2MASS J16024164+0131580
2MASS J16035008−1805459
2MASS J16041322+2331386
LHS 3149
2MASS J16045155−2104169
2MASS J16050179−2411327
2MASS J16062872−2003571
LP 861−22
LHS 3154
2MASS J16072853−2407543
2MASS J16074449−2036030
2MASS J16075875−2441319
2MASS J16084309−1900519
2MASS J16090397−1939456
2MASS J16095933−1800090
2MASS J16100184−2349432
2MASS J16102152−1941318
2MASS J16102639−1939513
LHS 3162
LP 684−33
2MASS J16111662−1939103
NLTT 42255
2MASS J16131023−1904131
G 153−36
LP 917−23
2MASS J16155487−2315146
2MASS J16162012−2344141
NLTT 42501
LP 445−8
WSB 10
1AXG J162356−2620
G 202−47
LHS 3196
GJ 3954
Table A2: (continued).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
817
818
819
820
821
822
823
824
825
826
827
828
829
830
831
832
833
834
835
836
837
838
839
840
841
842
843
844
845
846
847
848
849
850
851
852
853
854
855
856
857
858
859
860
861
862
863
864
162944.2−244121
162949.3+163624
163019.3+124955
163035.6+051020
163118.7+405152
163123.8+220741
163226.7−285312
163425.1+475028
163605.8−044013
163701.4+353543
164005.9+004218
164049.0−272521
164134.9+042711
164205.9−170958
164214.9+415942
164543.3+044440
164631.4+343453
165057.9+222706
165109.9+355507
165221.1+400619
165633.5−204638
165904.0+382259
170335.8+081814
170359.6+011423
170712.5+413644
170740.8+072206
171146.1+402901
171518.9+045750
171744.0+114011
171855.8+364223
171932.7−123005
171952.9+263003
172042.5+420506
172102.7+125844
172154.5+212547
172441.7+042248
172635.7+203125
172811.0−014357
173103.9+350408
173145.1+305604
173314.3+255704
173353.1+165512
173408.6−084952
173540.8+085641
173807.1−085537
174629.3−084237
175135.5+374936
175530.6−045542
−9.0
+27.3
−140.2
−213.8
−148.3
+16.9
+60.1
−477.7
−417.7
−197.3
+176.0
+51.7
−111.5
−323.1
−132.3
−86.0
−382.7
+30.3
−71.5
+22.3
−193.1
+70.2
−101.3
+0.5
−160.3
−493.5
+249.1
+578.4
−345.5
+64.1
−82.3
−234.1
+155.1
−247.9
−154.5
+143.1
−53.1
+100.4
−95.3
+35.2
−79.9
−108.6
−188.2
+61.8
−17.6
−37.6
−93.2
+66.8
−20.9
+22.5
−185.3
+24.9
+310.3
−156.4
−82.2
−55.0
−64.2
−509.9
−157.5
−185.7
−358.6
−421.4
−265.3
−470.9
−389.5
+397.1
+171.7
+201.2
−188.7
−30.4
−346.2
−0.7
+105.9
−375.2
+82.1
−746.2
−416.9
−409.5
−519.7
+358.5
−215.9
+136.1
+268.9
−192.8
−27.4
−159.7
+163.5
−225.2
−326.7
−133.1
−317.9
+20.6
−301.0
−424.6
+346.9
+40.0
14.455
13.596
15.044
15.245
14.073
15.123
14.746
14.847
15.493
15.898
13.056
15.720
15.629
15.316
14.525
15.274
15.951
13.426
14.297
15.187
16.593
15.380
15.454
13.710
14.792
13.439
15.098
14.086
14.405
15.317
15.407
12.342
13.840
15.347
13.248
15.189
15.595
13.858
14.856
14.962
15.279
13.700
15.240
14.969
15.532
12.194
15.433
14.600
10.082
9.589
10.925
11.332
9.461
11.187
10.791
10.743
11.053
11.135
9.116
11.479
11.497
11.123
10.500
10.713
10.533
9.136
10.334
11.267
11.299
11.058
11.374
9.275
10.690
9.284
11.074
9.750
9.817
11.374
11.273
8.229
9.895
11.064
9.344
10.794
11.044
9.889
10.863
10.926
11.272
8.895
10.905
10.871
11.100
8.198
10.442
10.696
9.144
8.777
10.035
10.476
8.506
10.337
9.970
9.862
10.183
10.240
8.209
10.589
10.636
10.244
9.618
9.791
9.606
8.309
9.488
10.466
10.368
10.190
10.490
8.407
9.826
8.419
10.271
8.782
8.931
10.533
10.453
7.351
9.000
10.170
8.492
9.847
10.140
9.010
9.959
10.067
10.387
7.995
10.055
10.015
10.180
7.353
9.496
9.784
2MASS J16294427−2441218
2MASS J16294932+1636245
NLTT 42951
NLTT 42959
GJ 3959
2MASS J16312383+2207426
1RXS J163226.4−285313
LHS 6308
LP 685−36
LHS 3227
GJ 3967
2MASS J16404898−2725204
NLTT 43373
LHS 3237
G 203−21
LHS 5321
LHS 3241
GJ 3976
LP 276−29
LP 226−3
2MASS J16563362−2046373
2MASS J16590404+3822593
2MASS J17033581+0818146
V* V371 Oph
LP 226−38
GJ 1210
G 203−50
GJ 1214
LHS 3277
2MASS J17185585+3642246
2MASS J17193275−1230032
Ross 867
G 203−60
LP 507−15
GJ 4003
NLTT 44733
NLTT 44801
2MASS J17281105−0143569
2MASS J17310397+3504074
LP 332−33
NLTT 45038
2MASS J17335314+1655129
LP 688−3
[SLS2012] PYC J17356+0856
LP 688−8
Wolf 1473
LP 278−42
2MASS J17553063−0455424
63
Table A2: (continued).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
865
866
867
868
869
870
871
872
873
874
875
876
877
878
879
880
881
882
883
884
885
886
887
888
889
890
891
892
893
894
895
896
897
898
899
900
901
902
903
904
905
906
907
908
909
910
911
912
175549.7+384213
175652.1+190555
180233.9+363045
180246.2+373101
180918.0+270626
181152.2+322521
181155.4+322547
181534.7+395259
181835.4−371013
182757.8+372416
183055.2+473601
183202.9+203057
183948.4+164849
184107.0−375011
184237.1+311105
184607.4−325008
185233.7+453833
185639.7−370721
185659.2−401143
190201.0+411403
190712.7+441607
191228.1+382615
191306.1−231206
191731.5+283314
191941.0+412748
192434.9−344239
192752.7−281117
193104.6−030617
193530.4−072940
193823.3+002104
194212.8−204548
194307.3+451810
194453.9−233800
194822.5−082253
195354.5+442452
195723.7−123351
195751.8−105305
200428.4−335611
200430.8−234204
200457.0+032107
201040.2+404008
201055.5−253512
201117.4−291758
201249.3−313024
201259.9+011258
201314.0+150031
201455.5+394326
201741.2−182036
−293.7
−242.2
−86.9
+180.1
+58.3
−150.5
−153.4
+15.4
−32.8
−3.0
−26.2
−50.7
+135.1
+6.9
−238.3
+20.2
+208.2
−0.2
+20.2
+34.4
+116.1
+280.3
+167.9
−2.9
+82.8
+20.8
+63.0
+207.2
−2.6
−10.0
−12.5
+122.2
+319.6
−445.5
+49.3
−92.4
−395.0
+74.9
+128.3
−102.8
+295.9
+5.4
+104.7
+178.8
−12.3
−3.7
−4.9
+219.8
+33.8
−216.2
−242.0
−1139.2
+226.7
+326.1
+322.6
−147.8
−114.3
+335.5
+330.9
−208.3
−96.8
−5.9
−328.9
−131.6
+466.8
−24.5
−205.4
+210.9
+172.0
−180.3
−357.4
−220.9
−187.8
−65.8
−97.7
+478.8
−18.1
−1.3
−134.0
+269.3
−167.3
−379.2
−507.0
−522.6
−291.9
−105.8
−342.8
−332.1
−92.5
+3.4
−81.5
−412.9
+65.7
−4.2
−136.4
−155.0
15.611
14.866
15.161
14.257
14.407
14.872
15.945
14.644
13.949
15.244
15.760
14.569
16.219
10.035
15.228
15.919
14.419
16.281
14.784
15.576
14.592
16.069
16.339
15.331
16.069
13.653
14.215
16.100
13.450
14.803
13.597
16.256
13.442
15.866
12.801
14.770
13.743
13.982
12.468
14.559
14.755
14.214
15.604
14.452
15.114
12.614
14.447
15.479
11.473
10.625
11.077
9.720
10.461
10.885
11.498
10.665
9.778
11.182
11.258
10.653
11.425
5.909
11.152
11.429
10.493
10.990
10.607
11.411
10.447
11.201
11.434
10.758
11.259
9.670
9.687
11.147
8.640
9.829
9.598
11.331
9.169
11.120
7.791
10.212
9.730
10.042
8.559
10.052
10.795
10.217
10.937
10.481
10.486
8.577
10.297
11.468
10.591
9.740
10.251
8.887
9.572
10.024
10.581
9.812
8.924
10.337
10.384
9.756
10.528
4.998
10.273
10.549
9.673
10.046
9.729
10.513
9.559
10.311
10.516
9.923
10.374
8.785
8.786
10.228
7.672
9.004
8.756
10.380
8.265
10.191
6.854
9.318
8.843
9.170
7.701
9.181
9.941
9.352
10.015
9.572
9.585
7.613
9.457
10.571
LP 278−50
2MASS J17565213+1905558
LP 278−58
LHS 457
NLTT 46025
G 206−16
NLTT 46103
2MASS J18153472+3953004
[SZB2012] 103
LP 279−37
LP 182−4
LSPM J1832+2030S
2MASS J18394841+1648497
V* U CrA
G 206−41
2MASS J18460763−3250107
LHS 3420
2MASS J18563974−3707205
2MASS J18565922−4011415
2MASS J19020105+4114024
LP 230−29
2MASS J19122805+3826161
2MASS J19130608−2312052
2MASS J19173151+2833147
LP 230−40
2MASS J19243494−3442392
LHS 5348
2MASS J19310458−0306186
TYC 5156−662−1
64
2MASS J19421282−2045477
2MASS J19430726+4518089
LP 869−26
2MASS J19482268−0822520
** GIC 159
GJ 773 B
LP 754−8
2MASS J20042845−3356105
LP 870−65
2MASS J20045709+0321076
G 209−18
LHS 3528
2MASS J20111744−2917584
LP 926−43
2MASS J20125995+0112584
V* V586 Aql
2MASS J20145550+3943272
LP 814−43
Table A2: (continued).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
913
914
915
916
917
918
919
920
921
922
923
924
925
926
927
928
929
930
931
932
933
934
935
936
937
938
939
940
941
942
943
944
945
946
947
948
949
950
951
952
953
954
955
956
957
958
959
960
201902.8+220521
201909.2+143816
202214.6+403002
202235.8−122254
202322.1+080014
202438.7+393030
202616.4+373301
202910.5+160120
202948.3+094120
202958.6+205434
203001.9+002355
203235.3+355835
203238.4+404044
203243.8+404217
203256.4+411207
203302.9+404725
203311.2+404233
203315.7+282344
203337.6−255652
203346.7−373345
203417.1+410630
203817.1+402105
203846.0−210645
204033.9+152959
204110.9+180005
204147.4+493848
204245.2−050018
204323.9+044555
204522.1+350815
204611.9+221956
205113.6−132916
205231.4−014709
205309.1−013304
205323.8−041637
205333.0+103701
205500.8+035529
205912.6−342735
210009.0+433108
210133.3+395703
210246.1+345435
210251.5−070248
210312.9+220832
210343.5+171648
210435.5+021159
210603.2+221848
210616.6+443702
210954.6+472904
211004.6−192030
−3.6
−84.6
−34.7
−4.5
+30.0
−4.0
−402.5
−56.4
+697.6
−133.6
+120.5
+126.7
−1.7
−2.2
−0.4
−0.9
−19.3
−247.5
+55.4
+76.1
−2.7
−2.0
−206.8
+1320.4
+143.1
+157.5
+233.9
+465.5
+376.6
+158.4
+651.2
−88.8
+354.6
+190.9
−490.8
+42.1
+289.9
+133.6
−151.0
+235.3
+78.7
+170.9
+208.0
−17.4
−21.2
−26.8
+417.9
+83.8
+3.6
−341.8
−14.7
+2.9
−225.3
−4.3
+358.6
+148.9
+209.9
−214.0
+11.1
+119.1
−3.5
−2.9
−1.6
−2.6
−1.1
−295.5
−75.3
−112.4
−2.6
−6.3
+60.3
+657.4
+61.4
+50.5
+110.9
−146.7
+122.5
+35.0
−170.8
−53.5
−218.7
−442.9
−448.7
−82.1
−244.4
+13.0
+7.5
−253.7
−56.7
+63.8
+21.1
−316.9
−198.2
−135.0
+153.9
−91.2
12.217
15.736
10.537
10.423
14.518
13.179
14.353
15.285
12.496
14.981
13.904
15.304
12.406
14.168
15.050
11.449
13.072
13.904
14.251
15.756
14.191
14.057
15.331
12.778
16.022
14.772
16.721
14.687
14.838
15.315
15.566
15.005
15.044
15.738
13.343
15.533
15.431
15.860
15.470
13.990
15.102
15.403
14.961
15.408
15.970
15.239
15.802
12.524
7.333
11.440
6.590
5.991
10.318
9.213
10.409
11.258
8.228
11.051
9.911
11.340
8.347
10.231
11.074
7.251
9.084
9.963
9.712
10.848
10.121
10.046
10.973
8.641
11.331
10.416
11.449
10.083
10.497
11.399
11.424
10.896
10.659
11.420
9.348
11.498
11.349
11.292
10.990
9.846
11.135
11.356
10.976
11.386
11.311
10.969
11.487
8.428
6.399
10.588
5.600
5.127
9.407
8.247
9.440
10.382
7.307
10.199
9.093
10.493
7.383
9.292
10.092
6.274
8.105
9.097
8.877
9.957
9.141
9.098
10.115
7.749
10.422
9.541
10.539
9.136
9.623
10.528
10.612
10.070
9.793
10.549
8.481
10.669
10.490
10.377
10.116
9.001
10.256
10.477
10.095
10.432
10.377
10.128
10.633
7.552
HD 346301B
LP 515−4
TYC 3156−1652−1
HD 193802
2MASS J20232212+0800149
2MASS J20243873+3930300
2MASS J20261645+3733012
2MASS J20291058+1601202
GJ 791.2
2MASS J20295868+2054344
I20300+0023
2MASS J20323532+3558353
[CPR2002] A25
SDSS J203243.87+404217.1
2MASS J20325647+4112075
[CPR2002] A20
[CPR2002] A22
G 210−26
2MASS J20333759−2556521
2MASS J20334670−3733443
2MASS J20341716+4106305
2MASS J20381712+4021059
LP 871−38
LHS 495
2MASS J20411094+1800050
2MASS J20414744+4938482
LP 695−372
LHS 5358
2MASS J20452209+3508146
2MASS J20461188+2219562
2MASS J20511351−1329161
LP 636−16
2MASS J20530910−0133039
LP 696−13
LHS 3593
[SLS2012] PYC J20550+0355
2MASS J20591244−3427335
65
2MASS J21013344+3957037
G 211−9
2MASS J21025150−0702487
2MASS J21031292+2208318
G 144−57
NLTT 50464
2MASS J21060322+2218480
2MASS J21095447+4729043
BPS CS 22898−0066
Table A2: (continued).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
961
962
963
964
965
966
967
968
969
970
971
972
973
974
975
976
977
978
979
980
981
982
983
984
985
986
987
988
989
990
991
992
993
994
995
996
997
998
999
1000
1001
1002
1003
1004
1005
1006
1007
1008
211031.0−271052
211031.5−271058
211113.6−224819
211124.1−094034
211540.8+165716
211807.1+482812
212133.8−243322
212243.0+085325
212336.2−261400
212342.7+271236
212432.4+400400
212700.8+351801
212923.3−185509
212953.9+491843
213118.8−094726
213429.4−184037
213517.5+463315
213627.2+250009
213740.1+013713
214146.9−270456
214225.2−262405
214229.6+232912
214309.8+074504
214407.9+170437
214717.4−044440
214901.7+015646
214932.7−073801
215009.3+055810
215127.0−012714
215148.3+133615
215311.9−255957
215517.4−004547
215524.2−023824
215619.7−102017
215655.2−015409
215712.7−090327
215814.4−210427
220118.3+434820
220421.5+150552
220509.4−124046
220609.7−072337
220748.5+053910
220850.3+114413
221124.1+405958
221203.5+164108
221554.8+232101
221636.4+131122
221736.4−114521
+64.6
+43.0
−41.1
−31.0
+39.7
+2.1
−95.1
+259.4
+37.7
+155.5
+545.4
+207.5
−33.2
−0.7
+28.3
+80.5
−163.1
+254.0
+77.3
+142.6
−39.7
+3.9
+421.3
+258.6
+245.3
+129.3
+155.7
+151.0
+213.5
+173.4
−431.4
+64.5
+154.5
−305.1
+1280.2
+176.1
+205.8
+21.8
+647.1
+374.6
+175.3
+457.1
+90.5
−89.6
+463.6
−111.8
+175.0
+8.2
−69.3
−58.5
−342.4
−343.5
−17.4
−2.8
−27.3
−273.8
−272.7
+78.9
+441.0
−8.4
−185.6
−6.6
−218.1
−15.4
−415.6
+107.6
−65.6
−274.7
−309.1
−357.0
−14.5
−6.2
−10.6
+91.0
−79.4
−17.1
+19.0
−118.2
−17.8
−53.7
+30.9
−261.2
+615.9
−124.8
−30.5
−22.8
+503.5
−148.4
−217.0
+120.4
−50.9
+68.0
−69.4
−193.3
+89.7
−17.7
16.213
14.624
14.064
15.791
15.294
15.277
15.066
15.378
15.164
15.785
15.272
15.467
16.105
15.356
11.390
14.076
15.421
15.153
12.788
14.963
15.691
15.343
15.747
14.301
13.504
15.251
15.712
14.755
16.237
13.275
16.054
15.172
14.820
13.920
14.066
14.428
15.437
14.715
15.651
15.124
15.537
15.462
13.869
14.371
15.663
16.082
15.309
15.644
11.200
10.296
9.987
10.937
11.342
11.264
11.061
11.407
11.226
11.427
10.339
11.484
11.263
10.909
7.316
10.046
11.297
11.003
8.802
10.699
11.321
11.211
11.325
10.078
9.416
11.340
11.473
10.657
11.282
9.311
11.479
11.092
10.663
9.925
9.880
10.142
11.444
10.530
10.867
10.981
10.674
11.155
9.901
9.725
11.431
10.985
11.364
11.421
10.236
9.411
9.121
9.950
10.491
10.279
10.183
10.598
10.355
10.524
9.431
10.641
10.301
10.077
6.379
9.188
10.460
10.159
7.884
9.786
10.465
10.305
10.506
9.193
8.501
10.451
10.617
9.771
10.385
8.423
10.593
10.197
9.809
9.086
9.026
9.239
10.611
9.642
9.981
10.147
9.759
10.242
9.037
8.790
10.556
10.115
10.545
10.549
2MASS J21103096−2710513
2MASS J21103147−2710578
LP 873−9
LP 757−92
2MASS J21154087+1657161
IRAS 21163+4815
2MASS J21213394−2433226
NLTT 51136
LP 873−38
2MASS J21234270+2712357
2MASS J21243234+4003599
2MASS J21270079+3518011
LP 817−54
Cl* NGC 7092 PLAT 2080
Wolf 922
2MASS J21342935−1840372
LHS 6379
2MASS J21362714+2500088
GSC 00543−00620
LP 930−22
LP 874−18
NLTT 51901
NLTT 51917
G 126−30
PM I21472-0444
NLTT 52157
LP 698−49
2MASS J21500933+0558102
LP 638−50
LP 518−58
LP 874−37
2MASS J21551741−0045478
2MASS J21552420−0238247
LP 758−62
LHS 516
LP 759−6
LP 874−66
2MASS J22011804+4348240
2MASS J22042147+1505517
LP 759−23
LP 699−32
LHS 5381
PM I22088+114
2MASS J22112417+4059587
2MASS J22120345+1641093
NLTT 53354
LP 519−50
UCAC3 157−291252
66
Table A2: (continued).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
1009
1010
1011
1012
1013
1014
1015
1016
1017
1018
1019
1020
1021
1022
1023
1024
1025
1026
1027
1028
1029
1030
1031
1032
1033
1034
1035
1036
1037
1038
1039
1040
1041
1042
1043
1044
1045
1046
1047
1048
1049
1050
1051
1052
1053
1054
1055
1056
221813.7−371350
222601.2−151813
222729.4+384724
223019.8+041010
223219.4−141835
223423.2−165945
223447.1+275754
223455.2+175201
223635.3−024050
224318.9−092742
224323.1−242453
224323.2+220818
224329.3+455514
224500.1−331526
224637.6+033248
224655.9+143714
224822.5+123210
224854.5+181958
224908.3−285121
225016.4−295217
225055.1+495913
225135.2−110406
225135.3−110407
225205.3−153250
225349.7−172135
225626.3−110937
225820.1+431255
225832.0+101458
225914.8+373639
230123.9−264946
230252.4+433815
230407.7−170757
230803.4+223251
230825.5+481338
231054.8+453045
231216.7+141427
231347.3+211729
231522.0−134619
231554.5−062746
232038.3+082110
232113.0+302309
232121.9+433807
232400.0+283403
232641.3−150431
232744.2−304540
233011.3−023722
233038.0−331827
233045.3+072627
+195.1
+277.3
+159.0
−121.0
−196.5
+501.3
−132.9
−428.9
−375.5
−60.3
+203.6
+390.0
+250.9
+173.2
+141.3
+336.3
+501.3
−24.7
−173.2
−278.1
+106.4
+359.8
+359.8
+338.4
+32.5
+391.2
+140.9
+163.9
+96.2
+262.3
−137.4
+256.3
+286.7
+163.6
−27.1
−127.7
+246.3
+301.9
+320.5
+26.3
+167.4
+196.0
+723.6
−43.3
+78.0
+101.7
−104.1
+485.5
−38.9
−49.0
+69.2
−289.6
−9.8
+0.9
−68.2
+12.8
−443.0
−219.8
−238.5
+1.3
−63.2
−125.3
−71.5
+53.2
−13.0
−132.8
−234.7
−393.0
−12.0
−145.7
−145.7
+11.4
+43.2
+272.5
−15.1
−169.3
−28.9
+30.2
−6.9
−260.4
+74.1
−129.2
−262.5
−95.3
−35.5
−256.5
−48.8
−125.4
+117.2
+59.8
−80.3
−87.1
−72.9
−77.3
−49.7
+267.5
15.764
16.326
15.155
14.611
15.249
15.733
15.661
15.676
15.767
15.903
14.299
14.315
14.826
12.740
15.351
15.816
16.178
13.897
13.300
15.342
13.859
14.400
14.575
14.369
15.201
14.410
15.389
14.980
14.638
14.669
13.264
15.405
14.725
15.094
15.586
15.115
16.124
14.696
16.337
15.114
14.610
15.719
15.216
13.933
14.493
15.090
14.288
15.003
11.410
11.456
11.251
10.518
11.227
11.231
11.192
11.415
11.416
11.498
10.250
10.143
10.902
8.681
11.376
11.418
11.193
9.957
9.342
11.281
9.804
9.996
9.996
10.236
11.188
10.496
11.211
10.391
10.378
10.739
9.316
11.477
10.681
11.098
10.844
10.908
11.421
10.737
11.111
10.843
10.630
11.457
10.920
9.986
10.486
10.648
10.184
10.821
10.509
10.561
10.374
9.688
10.351
10.317
10.367
10.583
10.548
10.635
9.408
9.258
10.028
7.793
10.491
10.521
10.232
9.119
8.474
10.448
8.920
9.130
9.130
9.370
10.318
9.626
10.319
9.499
9.535
9.881
8.453
10.638
9.745
10.163
9.896
10.060
10.443
9.903
10.228
9.885
9.802
10.581
10.058
9.112
9.664
9.768
9.317
9.974
LP 983−134
LP 820−19
NLTT 53909
NLTT 54021
LP 760−33
LHS 3831
2MASS J22344716+2757542
LP 460−43
LHS 3834
LP 760−66
LP 876−8
GJ 4292
2MASS J22432928+4555150
V* TX PsA
2MASS J22463761+0332484
LP 521−15
LHS 3856
2MASS J22485459+1819592
LP 932−83
LP 932−7
PM I22509+4959
CCDM J22516−1104P
CCDM J22516−1104A
LP 821−27
2MASS J22534969−1721358
LP 761−6
2MASS J22582006+4312551
NLTT 55442
2MASS J22591479+3736395
LP 933−37
2MASS J23025250+4338157
LP 821−55
G 128−33
2MASS J23082543+4813393
UCAC3 272−282107
2MASS J23121677+1414279
RX J2313.7+2117
LP 762−36
LP 702−50
SDSS J232038.38+082110.4
LP 346−8
LP 238−45
LHS 3940
UCAC3 150−396327
GR* 411
2MASS J23301129−0237227
GR* 422
LHS 3962
67
Table A2: (continued).
No.
CMC15
µα cos δ
[mas/a]
µδ
[mas/a]
r0
[mag]
J
[mag]
Ks
[mag]
Name
1057
1058
1059
1060
1061
1062
1063
1064
1065
1066
1067
1068
1069
1070
1071
1072
1073
1074
1075
1076
1077
1078
1079
1080
233144.9−024439
233147.6−062551
233201.3+005243
233541.3+061120
233607.5+105154
233623.7−104144
233736.0+162203
233910.6+305711
234022.3+343314
234139.4−063551
234252.6+304921
234400.7+224202
234437.5+304824
234617.0+133602
234619.3−115644
234720.6+423809
234721.6−122036
234824.1+283434
235223.5−144125
235232.3−341307
235359.4+282815
235640.9−145230
235810.8+035323
235919.8+324123
+95.1
−27.7
−133.8
+555.1
+293.2
+240.5
+16.7
+253.3
+533.8
+284.8
−341.9
+214.2
+149.0
+160.4
+224.1
+12.9
−306.2
+366.1
+416.7
+137.4
+399.0
+214.3
+278.8
−175.0
−73.3
−164.1
−324.7
+270.1
−314.3
−91.8
+32.3
+58.8
+93.8
−93.0
−299.2
−292.4
+0.9
−243.1
−128.9
+208.0
−146.5
−48.1
−257.6
−135.3
+123.2
+72.9
+42.8
−245.8
13.888
13.860
15.411
15.443
15.414
14.769
15.333
15.738
15.269
14.518
13.766
15.640
15.209
15.425
15.097
15.498
15.194
15.261
14.679
15.509
14.641
14.082
15.894
14.518
9.507
9.844
11.230
11.088
11.197
10.654
10.479
11.200
10.572
10.323
9.637
11.444
11.198
11.465
10.665
10.947
10.675
11.320
10.436
11.310
10.568
9.998
11.462
10.451
8.667
8.907
10.355
10.169
10.339
9.772
9.616
10.286
9.681
9.396
8.814
10.582
10.383
10.564
9.755
10.121
9.763
10.425
9.554
10.422
9.731
9.110
10.583
9.555
V* AF Psc
2MASS J23314763−0625502
NLTT 57142
GJ 4345
NLTT 57353
G 273−80
LP 463−23
NLTT 57522
LHS 3997
LP 703−42
GJ 1288
LP 402−78
2MASS J23443752+3048248
LP 523−40
G 273−133
LP 239−52
2MASS J23472176−1220358
LP 347−12
LHS 4032
2MASS J23523223−3413068
G 130−21
G 273−177
NLTT 58585
G 130−31
68
Appendix B: Application for Observing Time
Attached the application for observing time of CAHA 2015 in an independent .pdf file.
69

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