A search for faint blue stars in high galactic latitudes. IV Star and quasar distribution as a function of the magnitude in the PHL and PB surveys near the South Galactic Pole

Details A search for faint blue stars in high galactic latitudes. IV Star and quasar distribution as a function of the magnitude in the PHL and PB surveys near the South Galactic Pole A search for faint blue stars in high galactic latitudes. IV Star and quasar distribution as a function of the magnitude in the PHL and PB surveys near the South Galactic Pole

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26as...61..191b&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 61, Aug. 1985, p. 191-202.

Astronomy and Astrophysics

Astronomy

5

Astronomical Catalogs, Blue Stars, Cosmology, Quasars, Southern Sky, Star Distribution, Ultraviolet Astronomy, Astronomical Photometry, Red Shift, Stellar Magnitude

Scientific paper

The PB survey and a part of the PHL survey, near the South Galactic Pole, are used to obtain the relationship between the cumulative count of UV-rich, starlike objects of classes I and II and their apparent magnitudes, averaged for a 36 square degree area. The corresponding relationship for quasars which appear like UV-rich objects of classes I and II, are obtained from the different models of the statistical evolution of quasars derived by Schmidt and Green. If the former and the latter relationships are combined, the percentages of the quasars and stars as a function of the apparent magnitude can be estimated.

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