Results of an astrometric experiment on the Crimea-Pushchino interferometer

Details Results of an astrometric experiment on the Crimea-Pushchino interferometer Results of an astrometric experiment on the Crimea-Pushchino interferometer

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984azh....61..375z&link_type=abstract

(Astronomicheskii Zhurnal, vol. 61, Mar.-Apr. 1984, p. 375-381) Soviet Astronomy (ISSN 0038-5301), vol. 28, Mar.-Apr. 1984, p. 2

Astronomy and Astrophysics

Astronomy

2

Astrometry, Radio Astronomy, Radio Interferometers, Signal To Noise Ratios, Stellar Oscillations

Scientific paper

The results of preliminary astrometric tests using the Crimea-Pushchino VLBI array, performed in July, 1981, are reported. The array comprises two identical RT-22 radio telescopes in a north-south orientation and separated by about 1200 km and has maximum angular resolution 2 marcsec; water-vapor emissions of Orion A, W49 N, and W51 MAIN in the 1.35-cm band are observed. The equatorial length of the baseline and the difference of the nominal frequencies of the local oscillators are corrected. Graphs and tables are provided.

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