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First-Year Wilkinson Microwave Anisotropy Probe (WMAP)* Observations: On-Orbit Radiometer Characterization

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N. Jarosik1, C. Barnes1, C. L. Bennett2, M. Halpern3, G. Hinshaw2, A. Kogut2, M. Limon2,4, S. S. Meyer5, L. Page1, D. N. Spergel6, G. S. Tucker2,4,7, J. L. Weiland8, E. Wollack2 and E. L. Wright9

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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.


Footnote
WMAP is the result of a partnership between Princeton University and the NASA Goddard Space Flight Center. The HEMT amplifiers used in WMAP were supplied by the National Radio Astronomy Observatory. Scientific guidance is provided by the WMAP Science Team.
Subject headings

cosmic microwave background; cosmology: observations; instrumentation: detectors; radio continuum: general; space vehicles: instruments


Dates

Issue 1 (2003 September)

Received 2003 February 11, accepted for publication 2003 March 19



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