Going towards the read-out of a 160 pixel FDM system for SAFARI 76 pixels connected R.A. Hijmering R. den Hartog J. van der Kuur J.R. Gao M. Ridder A.J. v/d Linden SPICA/SAFARI SPICA (JAXA/ESA) Infrared mission ~ 2.5m, ~8K mirror, Background limited Proposed for M5, launch in ~2028 to L2 Explores dusty area and find a route to habitable planets SAFARI instrument on SPICA (SRON + partners) 34-210μm Three band grating spectrometer S-band 2x10-19 W/√Hz 3400 TESs per band 2 FDM requirements for SPICA • • • • Pixels /channel 160 (22 channels) Detector resolution 0.2-0.4 aW/√Hz Signal band 60Hz crosstalk <0.2 10-4 Noise at SQUID input 10.5pA/√Hz Carrier frequency range 1-3MHz Carrier frequency spacing 12.5kHz Carrier frequency deviation 1.2kHz LC quality (Q) >2355f0(MHz)~7000 Using in house developed and fabricated superconducting LC filters In house developed TES arrays In house fabricated Front End Electronics and Demux Board And operated using in house developed software 3 FDM readout Circuit • • • • Each TES has its own LC filter with unique resonance frequency Multiple carries are send down at f0 to bias the individual TESs Signal from the TES creates an amplitude modulation read out via SQUID Demodulation at the resonance frequency reveals the signal • FDM read out assembly with flexible, superconducting connection to kilo-pixel TES detectors M. Bruijn (poster session 1 wednesday) • The development of frequency domain multiplexing readout of TES-based X-ray microcalorimeters for Athena H. Akamatsu (today) 4 2 coil Real Circuit 3 times voltage step down ~1M - Resistive 2/400Ω - Inductive 2/2000nH - Capacitive in LC 1:9 • 2 LC filters in unit cell high+low f0 • L gradiometric Main C • Bias C L div. 5 5 FDM readout electronics • • • • • DACbias supplied bias carriers Summed at SQUID amplifier Amplified by LNA ADC I and Q Remodulated send to input coil by DACfb for BBFB 6 First itteration of the 160 pixel FDM Changing Rstray off on step Stays normal Changing Rn Varying IVmin No step step • • • • • Loading at high R Varying Rn IV curves vary pixel to pixel Rn varies considerably Step features Switching neighbors on big effect Saturation power varies with f0 7 First itteration of the 160 pixel FDM Changing Rstray off on step Loading at high R Crosstalk! Changing Rn System not optimized against crosstalk Stays normal Varying IVmin No step Unable to read out 160 pixels simultaneously step Varying Rn • Mutual inductance: magnetic coupling between channels • Common impedance: impedance outside circuit acting as voltage divider • Carrier leakage: openess of filters for neighboring carriers 8 160V2-pixel experiment PTBC5 SQUID LC array TES array LC array LC filter chips: • 176 resonators (87% yield) • Spread over 2 chips • 1MHz-3.8MHZ GOALS ~160 pixels read out No effect of crosstalk High yield of TES+LC filters Variation of ∆f <2kHz TES limited noise No read out effects in TES characterisation TES bolometer array: • 176 TES +8R's (87% yield) • Tc : 107±3 mK • RN : 140 mΩ • Psat,design:20 fW @ 65 mK • NEPdesign: 7x10-19 W/√Hz 9 160 pixel experiment V2 • Reduction in wire bonds (Lcom↓) • Reduction in inductance division coils 5µH:50nH→2µH:20nH (Lcom↓) • Mounting in stages (¼ , ½, 1) coil Themometer Connection for coil Absorbing material Nb foil for shielding 10 160 pixel experiment V2 LC • • • • • • • 2 LC chips alternating f0 (M↓) Shuffling f0 (M↓) LC filter larger unit cell 3x3mm (M↓) Δf in unit cell >1MHz (M↓) Lcom total 6nH to 4.5nH, incl. SQUID L from 2 to 3µH (CL↓) factor 2 reduction Δf from 14 to 16kHz (CL↓) } rij/kolom 1 2 3 4 5 6 7 8 9 10 11 L1/H1 1 47 133 7 93 55 141 15 101 63 149 23 109 71 157 31 117 79 165 39 125 87 173 LC chip 1 L2/H2 2 3 89 51 137 11 97 59 145 19 105 67 153 27 113 75 161 35 121 83 169 43 129 3 45 135 5 95 53 143 13 103 61 151 21 111 69 159 29 119 77 167 37 127 85 175 odd 4 1 91 49 139 9 99 57 147 17 107 65 155 25 115 73 163 33 123 81 171 41 131 11 160 pixel experiment V2 TES • • • • • • Wet etch procedure Detector chip is smaller+symmetric Wiring shorter (M↓) Coplanar wiring further apart (M↓) Extra resistors for mapping Wiring 24mm ± 0.1mm=120Hz Development of ultra low noise TES bolometer arrays T. Suzuki (Talk Monday) 12 Measured results with one LC filter • Connected 38 pixels followed by 76 pixels • All TES' and R's connected found • 76 Q's between 20k and 60k • 76 ESR between 0.8 and 1.2 m; <ESR> = 1.0 m 13 Resonance frequencies • • • 7 frequencies with multiple seperation due to disconnected pixels Variation in ∆f up to 10kHz → -0.1 to 0.4% of f0 Variation in f0 caused by lithographic tolerances, first suspect is dielectric of capacitors 14 Reduction in crosstalk common impedance dL The measured common impedance is 1.5nH 4.5nH is expected and the difference is due to the screening of the input coil by the feedback coil in the SQUID 15 Crosstalk: effect of neighbors 90 80 70 60 50 100 120 140 160 180 Switching on neighbors has no effect on the IV curves or Power Plateaus No influence of neighbors, no noticeable electrical crosstalk 16 TES measurements • • • • Power Plateaus vary factor 2 due to lithographic tolerance and production issues with wet-etch DRIE process enables higher fabrication accuracy, ultra low noise ~40% No frequency dependent results, (caused by biasing circuit) Detector noise not electronic noise limited Fabrication of low noise TES array for the SAFARI instrument on SPICA M. Ridder (Poster G1.16 today) 17 Conclusions • • • • • Significant reduction in electrical crosstalk Close to high yield of TES and LC filters (87%) Frequency separation up to 10kHz >2kHz Device limited noise No read-out effects in device measurements as f0 dependent results 18
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