The Cross‐Correlation between Galaxies of Different Luminosities and Colors
Author(s) -
Yu Wang,
Xiaohu Yang,
H. J. Mo,
Frank C. van den Bosch
Publication year - 2007
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/519245
Subject(s) - astrophysics , physics , galaxy , autocorrelation , luminosity , correlation , correlation function (quantum field theory) , luminosity function , statistics , mathematics , geometry , optoelectronics , dielectric
We study the cross-correlation between galaxies of different luminosities andcolors, using a sample selected from the SDSS Dr 4. Galaxies are divided into 6samples according to luminosity, and each of these samples is divided into redand blue subsamples. Projected auto-correlation and cross-correlation isestimated for these subsample. At projected separations r_p > 1\mpch, allcorrelation functions are roughly parallel, although the correlation amplitudedepends systematically on luminosity and color. On r_p < 1\mpch, the auto- andcross-correlation functions of red galaxies are significantly enhanced relativeto the corresponding power laws obtained on larger scales. Such enhancement isabsent for blue galaxies and in the cross-correlation between red and bluegalaxies. We esimate the relative bias factor on scales r > 1\mpch for eachsubsample using its auto-correlation function and cross-correlation functions.The relative bias factors obtained from different methods are similar. For bluegalaxies the luminosity-dependence of the relative bias is strong over theluminosity range probed (-23.0
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom