Relative bias parameters from angular correlations of optical and IRAS galaxies

Details Relative bias parameters from angular correlations of optical and IRAS galaxies Relative bias parameters from angular correlations of optical and IRAS galaxies

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...350..119l&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 350, Feb. 10, 1990, p. 119-124. Research supported by the Israeli Academy o

Astronomy and Astrophysics

Astronomy

53

Angular Correlation, Galactic Clusters, Infrared Sources (Astronomy), Visual Observation, Autocorrelation, Cross Correlation, Infrared Astronomy Satellite

Scientific paper

The galaxy distributions in the optical catalogs UGC and ESO are compared with those in the IRAS sample by calculating the auto- and cross-angular correlation functions. It is found that each angular correlation function is well approximated by the form w(theta) = A (theta exp 1-gamma) out to an angular distance of 5 deg, with gamma = 1.7.

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