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An Absolute Measurement of the Cosmic Microwave Background Radiation Temperature at 10.7 GH[CLC]z[/CLC]
Author(s) -
Suzanne T. Staggs,
N. Jarosik,
S. S. Meyer,
David T. Wilkinson
Publication year - 1996
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/310388
Subject(s) - radiometer , cosmic microwave background , microwave radiometer , physics , optics , microwave , radiation , horn antenna , antenna (radio) , remote sensing , radiation pattern , geology , slot antenna , quantum mechanics , anisotropy , telecommunications , computer science
A balloon-borne experiment has measured the absolute temperature of thecosmic microwave background radiation (CMBR) at 10.7 GHz to be Tcmbr = 2.730 +-.014 K. The error is the quadratic sum of several systematic errors, withstatistical error of less than 0.1 mK. The instrument comprises a cooledcorrugated horn antenna coupled to a total-power radiometer. A cryogenicmechanical waveguide switch alternately connects the radiometer to the horn andto an internal reference load. The small measured temperature difference (<= 20mK) between the sky signal and the reference load in conjunction with the useof a cold front end keeps systematic instrumental corrections small.Atmospheric and window emission are minimized by flying the instrument at 24 kmaltitude. A large outer ground screen and smaller inner screen shield theinstrument from stray radiation from the ground and the balloon. In-flighttests constrain the magnitude of ground radiation contamination, and low levelinterference is monitored through observations in several narrow frequencybands.Comment: 14 pages, 1 figure, submitted to ApJ

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