BOOMERANG: A balloon-borne millimeter-wave telescope and total power receiver for mapping anisotropy in the cosmic microwave background

被引:68
作者
Crill, BP
Ade, PAR
Artusa, DR
Bhatia, RS
Bock, JJ
Boscaleri, A
Cardoni, P
Church, SE
Coble, K
de Bernardis, P
de Troia, G
Farese, P
Ganga, KM
Giacometti, M
Haynes, CV
Hivon, E
Hristov, VV
Iacoangeli, A
Jones, WC
Lange, AE
Martinis, L
Masi, S
Mason, PV
Mauskopf, PD
Miglio, L
Montroy, T
Netterfield, CB
Paine, CG
Pascale, E
Piacentini, F
Polenta, G
Pongetti, F
Romeo, G
Ruhl, JE
Scaramuzzi, F
Sforna, D
Turner, AD
机构
[1] CALTECH, Observ Cosmol, Pasadena, CA 91125 USA
[2] Cardiff Univ, Dept Phys & Astron, Cardiff CF24 3YB, S Glam, Wales
[3] Jet Prop Lab, Pasadena, CA USA
[4] CNR, IROE, I-50127 Florence, Italy
[5] ENEA, Frascati, Italy
[6] Stanford Univ, Dept Phys, Palo Alto, CA 94304 USA
[7] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
[8] Adler Planetarium & Astron Museum, Chicago, IL USA
[9] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy
[10] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA
[11] CALTECH, Ctr Infrared Proc & Anal, Pasadena, CA 91125 USA
[12] Queen Mary Univ London, London E1 4NS, England
[13] Univ Toronto, Dept Astron, Toronto, ON M5S 3H8, Canada
[14] Ist Nazl Geofis, I-00161 Rome, Italy
[15] Case Western Reserve Univ, Dept Phys, Cleveland, OH 44106 USA
关键词
balloons; cosmic microwave background; instrumentation : miscellaneous;
D O I
10.1086/376894
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We describe BOOMERANG, a balloon-borne microwave telescope designed to map the cosmic microwave background at a resolution of 10' from the Long Duration Balloon (LDB) platform. The millimeter-wave receiver employs new technology in bolometers, readout electronics, cold reimaging optics, millimeter-wave filters, and cryogenics to obtain high sensitivity to cosmic microwave background anisotropy. Sixteen detectors observe in four spectral bands centered at 90, 150, 240, and 410 GHz. The wide frequency coverage, the long-duration flight, the optical design, and the observing strategy provide strong rejection of systematic effects. We report the flight performance of the instrument during a 10.5 day stratospheric balloon flight launched from McMurdo Station, Antarctica, that mapped similar to2000 square degrees of the sky.
引用
收藏
页码:527 / 541
页数:15
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