A medium-scale measurement of the cosmic microwave background at 3.3 millimeters

Abstract

view Abstract Citations (90) References (9) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS A Medium-Scale Measurement of the Cosmic Microwave Background at 3.3 Millimeters Meinhold, Peter ; Lubin, Philip Abstract We have developed a system for making measurements of spatial fluctuations in the cosmic microwave background radiation, on an angular scale of 5' to a few degrees. The system consists of an off- axis Gregorian telescope with a nearly Gaussian response with full width at half-maximum (FWHM) adjustable from 20' to 50', a superconductor-insulator-superconductor (SIS) coherent receiver operating at 3.3 mm, and a pointing system capable of better than 1' RMS stabilization. We report on results from the system's first balloon flight in 1988 August, and ground-based measurements made from the South Pole in 1988 December. We use a portion of the South Pole data to place a 95% confidence level upper limit of {DELTA}T/T < 3.5 x 10^-5^ for Gaussian sky fluctuations in the background radiation at 20' angular scale and a limit of {DELTA}T/T < 3.3 x 10^-5^ on overall excess intrinsic sky noise. We also estimate dust contamination in our cosmic background radiation data using measurements of the Galaxy from this flight and a previous one, along with the IRAS 100 micron map. These anisotropy results give the most stringent limits on cold dark matter theories to date. Publication: The Astrophysical Journal Pub Date: March 1991 DOI: 10.1086/185965 Bibcode: 1991ApJ...370L..11M Keywords: Galactic Evolution; Radiation Measurement; Relic Radiation; Astronomical Models; Cosmic Dust; Emission Spectra; Spatial Distribution; Astrophysics; COSMIC BACKGROUND RADIATION; COSMOLOGY; EARLY UNIVERSE full text sources ADS |