A MEASUREMENT OF THE TEMPERATURE OF THE COSMIC MICROWAVE BACKGROUND AT A FREQUENCY OF 7.5 GHZ

被引:21
|
作者
KOGUT, A
BENSADOUN, M
DEAMICI, G
LEVIN, S
SMOOT, GF
WITEBSKY, C
机构
[1] UNIV CALIF BERKELEY, BERKELEY, CA 94720 USA
[2] UNIV CALIF BERKELEY LAWRENCE BERKELEY LAB, BERKELEY, CA 94720 USA
[3] UNIV CALIF BERKELEY, SPACE SCI LAB, BERKELEY, CA 94720 USA
来源
ASTROPHYSICAL JOURNAL | 1990年 / 355卷 / 01期
关键词
Cosmic background radiation; Earth: atmospheres;
D O I
10.1086/168745
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have measured the intensity of the cosmic microwave background (CMB) at a frequency of 7.5 GHz (wavelength 4.0 cm) using a ground-based, total power radiometer calibrated at the antenna aperture by an external cryogenic reference target. The radiometer measured the difference in antenna temperature between the reference target and the zenith sky from a dry, high-altitude site. Subtraction of foreground signals (primarily atmospheric and galactic emission) measured with the same instrument leaves the CMB as the residual. The radiometer measured the atmospheric antenna temperature by correlating the signal change with the air mass in the beam during tip scans. The small galactic signal was subtracted based on extrapolation from lower frequencies and was checked by differential drift scans. The limiting uncertainty in the CMB measurement was the effect of ground radiation in the antenna sidelobes during atmospheric measurements. The thermodynamic temperature of the CMB at 7.5 GHz is 2.60 ± 0.07 K (68% confidence level).
引用
收藏
页码:102 / 113
页数:12
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