A BOLOMETRIC MILLIMETER-WAVE SYSTEM FOR OBSERVATIONS OF ANISOTROPY IN THE COSMIC MICROWAVE BACKGROUND-RADIATION ON MEDIUM ANGULAR SCALES

被引:38
|
作者
FISCHER, ML
ALSOP, DC
CHENG, ES
CLAPP, AC
COTTINGHAM, DA
GUNDERSEN, JO
KOCH, TC
KREYSA, E
MEINHOLD, PR
LANGE, AE
LUBIN, PM
RICHARDS, PL
SMOOT, GF
机构
[1] UNIV CALIF BERKELEY,SPACE SCI LAB,BERKELEY,CA 94720
[2] UNIV CALIF SANTA BARBARA,DEPT PHYS,SANTA BARBARA,CA 93106
[3] NASA,GODDARD SPACE FLIGHT CTR,GREENBELT,MD 20771
[4] MAX PLANCK INST RADIOASTRON,W-5300 BONN,GERMANY
来源
ASTROPHYSICAL JOURNAL | 1992年 / 388卷 / 02期
关键词
COSMIC MICROWAVE BACKGROUND; INSTRUMENTATION PHOTOMETERS;
D O I
10.1086/171148
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the performance of a bolometric system designed to measure the anisotropy of the cosmic microwave background (CMB) radiation on angular scales from 0-degrees-3 to 3-degrees. The system represents a collaborative effort combining a low-background 1 m diameter balloon-borne telescope with new multimode feed optics, a beam modulation mechanism with high stability, and a four-channel bolometric receiver with passbands centered near frequencies of 3 (90), 6 (180), 9 (270), and 12 (360) cm-1 (GHz). The telescope has been flown three times with the bolometric receiver and has demonstrated detector noise limited performance capable of reaching sensitivity levels of DELTA-T/T(CMB) almost-equal-to 10(-5) with detectors operated at T = 0.3 K.
引用
收藏
页码:242 / 252
页数:11
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