Preliminary results of a galactic background survey at 45 MHz

Details Preliminary results of a galactic background survey at 45 MHz Preliminary results of a galactic background survey at 45 MHz

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981rmxaa...6...79b&link_type=abstract

(International Astronomical Union, Reunion Regional Latinoamericana de Astronomia, 2nd, Merida, Venezuela, Jan. 19-23, 1981) Rev

Astronomy and Astrophysics

Astronomy

3

Background Radiation, Galactic Radio Waves, Milky Way Galaxy, Radio Astronomy, Synchrotron Radiation, Angular Resolution, Radio Telescopes

Scientific paper

Preliminary results of a survey of the galactic background at 45 MHz recently carried out at the MaipuRadio Astronomy Observatory are shown. The radiotelescope is a transit instrument that consists of a rectangular filled array of 528 dipoles with an angular resolution of 2.1 deg in declination and 4.6 deg in righ ascension. These first observations cover the region of the sky between declinations from -30 deg to -37 deg and they have been obtained with a multiple beam system.

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