On estimates of the galaxy correlation function

Details On estimates of the galaxy correlation function On estimates of the galaxy correlation function

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.202.1245s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 202, Mar. 1983, p. 1245-1247.

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3

Angular Correlation, Astronomical Catalogs, Galaxies, Astronomical Photography, Data Reduction

Scientific paper

The form of the galaxy-galaxy angular correlation function obtained by Hewett (1982) is directly compared with the results of other investigators. It is determined that Hewett's result agrees closely with that of Shanks et al. (1980) who showed that a break in the correlation function's power-law behavior occurs at 3/h Mpc. It is concluded that independent analyses of machine measured data obtained from different UK Schmidt telescopes photographs seem to give very consistent galaxy angular correlation functions.

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