The angular correlation function of galaxies as a function of magnitude

Details The angular correlation function of galaxies as a function of magnitude The angular correlation function of galaxies as a function of magnitude

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apjs...62..301s&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 62, Oct. 1986, p. 301-330.

Astronomy and Astrophysics

Astrophysics

39

Angular Correlation, Astronomical Photometry, Galactic Clusters, Photographic Plates, Astronomical Photography, Classifications, Magnitude

Scientific paper

The scaling law of Peebles (1973) is extended and applied (with an automatic plate-scanning system and the faint-star/galaxy classifier and computer system described by Sebok, 1980) to determine the angular correlation function of apparent-magnitude-selected subcatalogs of galaxies from four red Palomar Schmidt-telescope plates of a 10-deg-sq area centered on alpha = 10 h, delta = 47 deg. The results are presented in tables and graphs and characterized in detail. The possibility of separating the effects of evolution from those of the spatial-correlation-function power-law slope is explored.

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