NOISE CORRELATIONS IN COSMIC MICROWAVE BACKGROUND EXPERIMENTS

被引:2
作者
DODELSON, S
KOSOWSKY, A
MYERS, ST
机构
[1] UNIV CHICAGO,ENRICO FERMI INST,DEPT PHYS,CHICAGO,IL 60637
[2] UNIV CHICAGO,ENRICO FERMI INST,DEPT ASTRON & ASTROPHYS,CHICAGO,IL 60637
[3] CALTECH,DIV PHYS MATH & ASTRON,PASADENA,CA 91125
关键词
COSMIC MICROWAVE BACKGROUND; METHODS; DATA ANALYSIS;
D O I
10.1086/187755
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Many analyses of microwave background experiments neglect the correlation of noise in different frequency or polarization channels. We show that these correlations, should they be present, can lead to severe misinterpretation of an experiment. In particular, correlated noise arising from either electronics or atmosphere may mimic a cosmic signal. We quantify how the likelihood function for a given experiment varies with noise correlation, using both simple analytic models and actual data. For a typical microwave background anisotropy experiment, noise correlations at the level of 1% of the overall noise can seriously reduce the significance of a given detection.
引用
收藏
页码:L37 / L39
页数:3
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