Isotropy of the cosmic background radiation at 3.4 millimeters with 10-arcsec resolution

Details Isotropy of the cosmic background radiation at 3.4 millimeters with 10-arcsec resolution Isotropy of the cosmic background radiation at 3.4 millimeters with 10-arcsec resolution

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...404l..33r&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 404, no. 2, p. L33-L35.

Astronomy and Astrophysics

Astrophysics

8

Background Radiation, Cosmic Rays, Isotropy, Radio Interferometers, Relic Radiation, Temperature Gradients, Brightness Temperature, Very Large Array (Vla)

Scientific paper

To search for angular fluctuations in the temperature of the cosmic background radiation, a high-declination blank fields was observed with the IRAM interferometer at a wavelength of 3.4 mm. The synthesized beam was 9 x 10 arcsec and the field of view 55 arcsec in diameter. At 95-percent confidence, the upper limit to any fluctuations in the image at this resolution is less than 900,000.

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