4.6 Article

Loose groups of galaxies in the Las Campanas Redshift Survey

Journal

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
Volume 130, Issue 2, Pages 237-265

Publisher

UNIV CHICAGO PRESS
DOI: 10.1086/317348

Keywords

catalogs; galaxies : clusters : general; galaxies : distances and redshifts; large-scale structure of universe; surveys

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A friends-of-friends percolation algorithm has been used to extract a catalog of deltan/n = 80 density enhancements (groups) from the six slices of the Las Campanas Redshift Survey (LCRS). The full catalog contains 1495 groups and includes 35% of the LCRS galaxy sample. A clean sample of 394 groups has been derived by culling groups from the full sample that either are too close to a slice edge, have a crossing time greater than a Hubble time, have a corrected velocity dispersion of zero, or contain a 55 orphan (a galaxy with a mock redshift that was excluded from the original LCRS redshift catalog due to its proximity to another galaxy-i.e., within 55 ). Median properties derived from the clean sample include a line-of-sight velocity dispersion sigma (los) = 164 km s(-1), crossing time t(cr), = 0.10 H-0(-1), harmonic radius R-h = 0.58 h(-1) Mpc, pairwise separation R-p = 0.64 h(-1) Mpc, virial mass M-vir = 1.90 x 10(13) h(-1) M., total group R-band luminosity L-tot = 1.30 x 10(11) h(-2) L., and R-band mass-to-light ratio M/L = 171 h M./L.; the median number of observed members in a group is three.

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