SHARC II: A Caltech Submillimeter Observatory facility camera with 384 pixels

被引:138
作者
Dowell, CD [1 ]
Allen, CA [1 ]
Babu, S [1 ]
Freund, MM [1 ]
Gardner, MB [1 ]
Groseth, J [1 ]
Jhabvala, M [1 ]
Kovacs, A [1 ]
Lis, DC [1 ]
Moseley, SH [1 ]
Phillips, TG [1 ]
Silverberg, R [1 ]
Voellmer, G [1 ]
Yoshida, H [1 ]
机构
[1] CALTECH, Pasadena, CA 91125 USA
来源
MILLIMETER AND SUBMILLIMETER DETECTORS FOR ASTRONOMY | 2003年 / 4855卷
关键词
submillimeter; instrumentation; bolometers;
D O I
10.1117/12.459360
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
SHARC II is a background-limited 350 mum and 450 mum facility camera for the Caltech Submillimeter Observatory undergoing commissioning in 2002. The key component of SHARC II is a 12x32 array of doped silicon 'pop-up' bolometers developed at NASA/Goddard. Each I mm x 1 mm. pixel is coated with a 400 Omega/square bismuth film and located lambda/4 above a reflective backshort to achieve >75% absorption efficiency. The pixels cover the focal plane with >90% filling factor. At 350 mum, the SHARC II pixels axe separated by 0.65 lambda/D. In contrast to the silicon bolometers in the predecessor of SHARC II, each doped thermistor occupies nearly the full area of the pixel, which lowers the 1/f knee of the detector noise to <0.03 Hz, under load, at the bath temperature of 0.36 K. The bolometers are AC-biased and read in 'total power' mode to take advantage of the improved stability. Each bolometer is biased through a custom similar to130 MOmega CrSi load resistor at 7 K and read with a commercial JFET at 120 K. The JFETs and load resistors are integrated with the detectors into a single assembly to minimize microphonic noise. Electrical connection across the 0.36 K to 4 K and 4 K to 120 K temperature interfaces is accomplished with lithographed metal wires on dielectric substrates. In the best 25% of winter nights on Mauna Kea, SHARC II is expected to have an NEFD at 350 mum of 1 Jy Hz(-1/2) or better. The new camera should be at least 4 times faster at detecting known point sources and 30 times faster at mapping large areas compared to the prior instrument.
引用
收藏
页码:73 / 87
页数:15
相关论文
共 23 条
[1]  
AMES TJ, 2002, P SPIE, V4848
[2]  
[Anonymous], DETECTION LIGHT ULTR
[3]   IMPROVED HE-3-HE-4 REFRIGERATOR [J].
DALLOGLIO, G ;
FISCHER, W ;
MARTINIS, L ;
PIZZO, L .
CRYOGENICS, 1993, 33 (02) :213-214
[4]  
DOWELL CD, 2002, CP211408 NASA
[5]  
FREUND MM, 2002, P SPIE, V4855
[6]  
GRIFFIN MJ, 2002, IN PRESS APPL OPT
[7]   Intrinsic l/f noise in doped silicon thermistors for cryogenic calorimeters [J].
Han, SI ;
Almy, R ;
Apodaca, E ;
Bergmann, W ;
Deiker, S ;
Lesser, A ;
McCammon, D ;
Rawlins, K ;
Kelley, RL ;
Moseley, SH ;
Porter, FS ;
Stahle, CK ;
Szymkowiak, AE .
EUV, X-RAY, AND GAMMA-RAY INSTRUMENTATION FOR ASTRONOMY IX, 1998, 3445 :640-644
[8]   HAWC - a far-infrared camera for SOFIA [J].
Harper, DA ;
Allen, C ;
Amato, M ;
Ames, T ;
Bartels, A ;
Casey, S ;
Derro, R ;
Evans, R ;
Gatley, I ;
Heimsath, S ;
Hermida, A ;
Jhabvala, M ;
Kastner, J ;
Loewenstein, RF ;
Moseley, SH ;
Pernic, RJ ;
Rennick, T ;
Rhody, H ;
Sandford, D ;
Shafer, R ;
Shirron, P ;
Voellmer, G ;
Wang, S ;
Wirth, J .
AIRBORNE TELESCOPE SYSTEMS, 2000, 4014 :43-53
[9]   SCUBA: a common-user submillimetre camera operating on the James Clerk Maxwell Telescope [J].
Holland, WS ;
Robson, EI ;
Gear, WK ;
Cunningham, CR ;
Lightfoot, JF ;
Jenness, T ;
Ivison, RJ ;
Stevens, JA ;
Ade, PAR ;
Griffin, MJ ;
Duncan, WD ;
Murphy, JA ;
Naylor, DA .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1999, 303 (04) :659-672
[10]   Optical design of the submillimeter high angular resolution camera (SHARC) [J].
Hunter, TR ;
Benford, DJ ;
Serabyn, E .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1996, 108 (729) :1042-1050