The Galaxy-Galaxy Autocorrelation Function for the Las Campanas Redshift Survey

Details The Galaxy-Galaxy Autocorrelation Function for the Las Campanas Redshift Survey The Galaxy-Galaxy Autocorrelation Function for the Las Campanas Redshift Survey

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aas...187.5406t&link_type=abstract

American Astronomical Society, 187th AAS Meeting, #54.06; Bulletin of the American Astronomical Society, Vol. 27, p.1365

Astronomy and Astrophysics

Astronomy

2

Scientific paper

The Las Campanas Redshift Survey (LCRS) is a galaxy survey which extends to a redshift of 0.2 and which is composed of a total of 6 alternating 1.5(deg) x 80(deg) Slices in the North and South Galactic Caps. Now in its final stages, the Survey contains approximately 26,400 galaxy redshifts. We present here a definitive LCRS galaxy-galaxy autocorrelation function xi_ ≫(s), its comparison to the xi_ ≫(s) from various theoretical models, and a discussion of the impact of the unique character of the LCRS galaxy selection criteria on the measurement of the observed xi_ ≫(s).

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