First-year Wilkinson Microwave Anisotropy Probe (WMAP) observations:: On-orbit radiometer characterization

被引:85
作者
Jarosik, N
Barnes, C
Bennett, CL
Halpern, M
Hinshaw, G
Kogut, A
Limon, M
Meyer, SS
Page, L
Spergel, DN
Tucker, GS
Weiland, JL
Wollack, E
Wright, EL
机构
[1] Dept Phys, Princeton, NJ 08544 USA
[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[3] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada
[4] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
[5] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
[6] Univ Chicago, Dept EFI, Chicago, IL 60637 USA
[7] Univ Chicago, Dept CFCP, Chicago, IL 60637 USA
[8] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
[9] Brown Univ, Dept Phys, Providence, RI 02912 USA
[10] Sci Syst & Applicat Inc, Lanham, MD 20706 USA
[11] Univ Calif Los Angeles, Dept Astron, Los Angeles, CA 90095 USA
关键词
cosmic microwave background; cosmology : observations instrumentation : detectors; radio continuum : general; space vehicles : instruments;
D O I
10.1086/377221
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The WMAP satellite has completed 1 year of measurements of the cosmic microwave background (CMB) radiation using 20 differential high electron mobility transistor (HEMT) based radiometers. All the radiometers are functioning nominally, and characterizations of the on-orbit radiometer performance are presented, with an emphasis on properties that are required for the production of sky maps from the time-ordered data. A radiometer gain model, used to smooth and interpolate the CMB dipole gain measurements, is also presented. No degradation in the sensitivity of any of the radiometers has been observed during the first year of observations.
引用
收藏
页码:29 / 37
页数:9
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