1/f noise and other systematic effects in the Planck-LFI radiometers

被引:66
作者
Seiffert, M
Mennella, A
Burigana, C
Mandolesi, N
Bersanelli, M
Meinhold, P
Lubin, P
机构
[1] CNR, IASF, Sez Milano, I-20133 Milan, Italy
[2] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[3] CNR, IASF, Sez Bologna, I-40126 Bologna, Italy
[4] Univ Milan, I-20133 Milan, Italy
[5] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA
关键词
cosmology : cosmic microwave background; observations; instrumentation : detectors; methods : analytical;
D O I
10.1051/0004-6361:20020880
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We use an analytic approach to study the susceptibility of the PLANCK Low Frequency Instrument radiometers to various systematic effects. We examine the effects of fluctuations in amplifier gain, in amplifier noise temperature and in the reference load temperature. We also study the effect of imperfect gain modulation, non-ideal matching of radiometer parameters, imperfect isolation in the two legs of the radiometer and back-end 1/f noise. We find that with proper gain modulation 1/f gain fluctuations are suppressed, leaving fluctuations in amplifier noise temperature as the main source of 1/f noise. We estimate that with a gain modulation factor within +/- 1% of its ideal value the overall 1/f knee frequency will be relatively small (<0.1 Hz).
引用
收藏
页码:1185 / 1197
页数:13
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