Log N-log S of radio sources at 10 GHz with flat spectra

Details Log N-log S of radio sources at 10 GHz with flat spectra Log N-log S of radio sources at 10 GHz with flat spectra

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.119..257a&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

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3

Astronomical Spectroscopy, Microwave Frequencies, Radio Sources (Astronomy), Computational Astrophysics, Luminosity, Space Density

Scientific paper

In order to study the log N-log S relation at 10 GHz, it is important to separate sources with flat spectra, such as compact QSOs, from those with steep spectra, which are primarily radio galaxies. Nobeyama Radio Observatory and other data are presently used to construct the log N-log S relation at 10 GHz for flat spectrum sources (alpha not greater than 0.5). On the basis of the source distribution on log (Luminosity) approximately equal to the volume plane, a luminosity function that is epoch-dependent is obtained to explain the relation.

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