Observational Bolometric
Lightcurves and SED's of Type Ia
Supernovae
Michael T. Smitka, Peter Brown, Nicholas Suntzeff
Texas A&M University
Data
UV
Optical
NIR
Photometry
SWIFT UVOT
CSP
CSP
Spectra
SWIFT UVOT
CSP
Marion, Hsiao
Status
We have all photometry in
hand.
CSP spectra are in prep.
I’m forming plans to reduce the
the UVOT spectra personally.
Some NIR spectra exist.
Goal
Produce time-series spectra
• spanning1600-25000Å
• -10d through 30d
Produce bolometric light curves
Produce what is useful to you.
2005cf
Bufano, 2009
Garavini, 2007
Gall, 2012
Hsiao, 2009