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The Las Campanas Redshift Survey Galaxy-Galaxy Autocorrelation Function
D. L. Tucker, A. Oemler, R. P. Kirshner +7
Presented are measurements of the observed redshift-space galaxy-galaxy autocorrelation function, xi(s), for the Las Campanas Redshift Survey (LCRS). For separations 2.0/h Mpc < s…
The Quadruple Gravitational Lens PG1115+080: Time Delays and Models
P. L. Schechter, C. D. Bailyn, R. Barr +24
Optical photometry is presented for the quadruple gravitational lens PG1115+080. A preliminary reduction of data taken from November 1995 to June 1996 gives component ``C'' leading…
The Power Spectrum of Galaxy Clustering in the Las Campanas Redshift Survey
Huan Lin, Robert P. Kirshner, Stephen A. Shectman +4
The Las Campanas Redshift Survey (LCRS) contains 23697 galaxies, with an average redshift , distributed over six $1.5\arcdeg$ by $80\arcdeg$ slices in the North and South…
The Las Campanas Redshift Survey
Stephen A. Shectman, Stephen D. Landy, Augustus Oemler +4
The Las Campanas Redshift Survey (LCRS) consists of 26418 redshifts of galaxies selected from a CCD-based catalog obtained in the band. The survey covers over 700 square degree…
The Luminosity Function of Galaxies in the Las Campanas Redshift Survey
Huan Lin, Robert P. Kirshner, Stephen A. Shectman +4
We present the -band luminosity function for a sample of 18678 galaxies, with average redshift , from the Las Campanas Redshift Survey. The luminosity function may be f…