Monte-Carlo simulations of galaxy systems. VI - The angular correlation function for faint galaxy samples

Details Monte-Carlo simulations of galaxy systems. VI - The angular correlation function for faint galaxy samples Monte-Carlo simulations of galaxy systems. VI - The angular correlation function for faint galaxy samples

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.105..331m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 105, no. 2, Oct. 1984, p. 331-337.

Statistics

Computation

1

Angular Correlation, Computational Astrophysics, Galactic Clusters, Monte Carlo Method, Astronomical Models, Mass Distribution

Scientific paper

The angular correlation function for the sample of faint galaxies described in MacGillivray and Dodd (1980), obtained from objective measures made with the COSMOS machine on a deep UKST photograph, is examined and compared with that for the model fields described in Paper V of this series (MacGillivray and Dodd, 1982). The results support the presence of clustering of galaxies in these machine-determined samples on scales up to 7 hr-1Mpc and are consistent with both the hierarchical and adiabatic schemes for galaxy clustering.

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