The RATAN-600 deep sky survey - Cooperative studies of 13h sources at Effelsberg, Zelenchukskaya, and Tonantzintla

Details The RATAN-600 deep sky survey - Cooperative studies of 13h sources at Effelsberg, Zelenchukskaya, and Tonantzintla The RATAN-600 deep sky survey - Cooperative studies of 13h sources at Effelsberg, Zelenchukskaya, and Tonantzintla

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..403w&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, June 1985, p. 403-414) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, May-June

Astronomy and Astrophysics

Astronomy

2

Astronomical Spectroscopy, International Cooperation, Radio Sources (Astronomy), Radio Telescopes, Sky Surveys (Astronomy), Mexico, Radiant Flux Density, Radio Galaxies, U.S.S.R., Visible Spectrum, West Germany

Scientific paper

Preliminary results are reported for a cooperative program (Mexico, Germany, USSR) to study the radio sources previously detected in the 7.6-cm RATAN-600 deep-sky surveys. Flux densities have been measured with the 100-m Effelsberg paraboloid at wavelengths of 6 and/or 11 cm for 19 RATAN-600 sources, and declinations have been refined for 13 objects. In the survey strip, the objects common to the RATAN-600 and Effelsberg surveys have a mean flux density of about 30 mJy; their positions are now accurate to 3 arcsec in alpha and 9 arcsec in delta. Three-frequency radio spectra are obtained for some sources brighter than 8 mJy. Many of the sources have been identified optically on glass copies of the Palomar Sky Survey.

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