The form of log N-log S relation in the domain of strong flux densities

Details The form of log N-log S relation in the domain of strong flux densities The form of log N-log S relation in the domain of strong flux densities

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.108..319a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 108, no. 2, Jan. 1985, p. 319-322.

Astronomy and Astrophysics

Astronomy

Radiant Flux Density, Radio Sources (Astronomy), Spectral Energy Distribution, Astronomical Models, Constraints, Universe

Scientific paper

The disparity between the slopes of log N-log S curves indicating the differential counts of radio sources at frequencies of hundreds of MHz in observations and those determined from models of the Universe is investigated analytically. Typical curves are shown, and it is demonstrated that the slope in the region of strong flux density is explained by placing a constraint on flux density and spectral-index spreading.

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