Title :
Tests of finline-coupled TES bolometers forCℓOVER
Author :
Audley, M.D. ; Glowacka, D.M. ; Goldie, D.J. ; Lasenby, A.N. ; Tsaneva, V.N. ; Withington, S. ; Grimes, P.K. ; North, C.E. ; Yassin, G. ; Piccirillo, L. ; Pisano, G. ; Ade, P.R. ; Teleberg, G. ; Irwin, K.D. ; Duncan, W.D. ; Reintsema, C.D. ; Halpern, M. ;
Author_Institution :
Cavendish Lab., Cambridge Univ., Cambridge
Abstract :
CLOVER aims to detect the signature of gravitational waves from inflation by measuring the B-mode polarization of the cosmic microwave background. CLOVER consists of two polarimeters. One operates at 97 GHz, using finline-coupled transition edge sensors (TES). The other has a combined 150/220-GHz focal plane populated by radial-probe coupled TES detectors. The 97-GHz instrument will have 100 feedhorns and 200 detectors while the combined 150 and 220-GHz instrument will have a total of 200 horns. To achieve the target NEP of 1.5 x 10-17 W Hz-1 the 97-GHz detectors will have a transition temperature of 190 mK and will operate with a base temperature of ~ 100 mK. CLOVER´s detectors are fabricated on 225-micron silicon substrates. In the 97-GHz instrument a finline transition feeds a microstrip which is terminated by a matched resistor on the silicon nitride island that carries the TES. Each detector is fabricated as a single chip to ensure a 100% operational focal plane. The detectors are mounted in linear modules made of copper which form split-block waveguides. Each detector module contains a time-division SQUID multiplexer to read out the detectors. The multiplexed signals are further amplified by SQUID series arrays. The first prototype detectors for CLOVER have a transition temperature of 350 mK and were fabricated to validate the detector design and the polarimeter technology. We have characterised these detectors in a dedicated test facility. The CLOVER testbed contains cryogenics similar to those in the final instrument: a pulse-tube cooler, He-7 sorption fridge, and a mini dilution fridge so that the detectors are tested in a realistic environment. The test bed has a cryogenic black- body source with band-defining filters for optical testing. As well as the multi-channel electronics that will be used on the final instrument the test bed has an analogue SQUID readout which allows us to characterise the readout fully. We discuss the resul- s of the detector tests and the design changes needed to achieve the required sensitivity.
Keywords :
SQUIDs; blackbody radiation; bolometers; gravitational wave detectors; microwave detectors; polarimeters; readout electronics; silicon; B-mode polarization measurement; CLOVER; SQUID series arrays; analogue SQUID readout; band-defining filters; cosmic microwave background; cryogenic black- body source; detector read out; finline transition; finline-coupled TES bolometers; finline-coupled transition edge sensors; frequency 150 GHz; frequency 220 GHz; frequency 97 GHz; gravitational waves signature; multi-channel electronics; optical testing; polarimeter technology; polarimeters; radial-probe coupled TES detectors; silicon substrates; size 225 micron; split-block waveguides; time-division SQUID multiplexer; Bolometers; Cryogenics; Detectors; Electronic equipment testing; Instruments; Microwave measurements; Optical filters; SQUIDs; Silicon; Temperature;
Conference_Titel :
Infrared and Millimeter Waves, 2007 and the 2007 15th International Conference on Terahertz Electronics. IRMMW-THz. Joint 32nd International Conference on
Conference_Location :
Cardiff
Print_ISBN :
978-1-4244-1438-3
DOI :
10.1109/ICIMW.2007.4516449