The Galaxy Correlation Function in the CNOC2 Redshift Survey: Dependence on Color, Luminosity, and Redshift

2001 ◽  
Vol 560 (1) ◽  
pp. 72-85 ◽  
Author(s):  
C. W. Shepherd ◽  
R. G. Carlberg ◽  
H. K. C. Yee ◽  
S. L. Morris ◽  
H. Lin ◽  
...  
Keyword(s):  
Correlation Function ◽  
The Galaxy ◽  
Redshift Survey

scholarly journals The Shane Wirtanen counts - Observability of the galaxy correlation function

1989 ◽  
Vol 338 ◽  
pp. 605 ◽  
Author(s):  
Michael E. Brown ◽  
Edward J. Groth
Keyword(s):  
Correlation Function ◽  
The Galaxy

scholarly journals Measuring the growth rate of structure around cosmic voids

2014 ◽  
Vol 11 (S308) ◽  
pp. 571-574
Author(s):  
A. J. Hawken ◽  
D. Michelett ◽  
B. Granett ◽  
A. Iovino ◽  
L. Guzzo
Keyword(s):  
Growth Rate ◽  
Correlation Function ◽  
Cross Correlation ◽  
Cross Correlation Function ◽  
Redshift Survey ◽  
Cosmic Voids

AbstractUsing an algorithm based on searching for empty spheres we identified 245 voids in the VIMOS Public Extragalactic Redshift Survey (VIPERS). We show how by modelling the anisotropic void-galaxy cross correlation function we can probe the growth rate of structure.

scholarly journals The Anglo-Australian Redshift Survey

1983 ◽  
Vol 104 ◽  
pp. 175-175
Author(s):  
J. Bean ◽  
G. Efstathiou ◽  
R. S. Ellis ◽  
B. A. Peterson ◽  
T. Shanks ◽  
...  
Keyword(s):  
Correlation Function ◽  
Luminosity Function ◽  
Large Scale ◽  
Peculiar Velocities ◽  
Point Correlation ◽  
Point Correlation Function ◽  
Redshift Survey ◽  
Density Inhomogeneities ◽  
The Universe

The aim of the survey is to sample a relatively large, randomly chosen volume of the Universe in order to study the large-scale distribution of galaxies using the two-point correlation function, the peculiar velocities between galaxy pairs and to provide an estimate of the galaxian luminosity function that is unaffected by density inhomogeneities and Virgo infall.

scholarly journals N-body Simulations to Test the Reliability of Two-point Correlation Functions of Galaxies

1992 ◽  
Vol 9 ◽  
pp. 703-704
Author(s):  
Yasushi Suto
Keyword(s):  
Correlation Functions ◽  
Large Scale ◽  
Sample Volume ◽  
Limited Data ◽  
Observable Universe ◽  
Large N ◽  
The Galaxy ◽  
Point Correlation ◽  
Systematic Biases ◽  
Redshift Survey

The shape and amplitude of the galaxy – galaxy correlation functions, ξgg(r), are among the most widely used measures of the large-scale structure in the universe (Totsuji & Kihara 1969). The estimates, however, might be seriously affected by the limited size of the sample volume, or equivalently, the limited number of available galaxies. In fact, while the observable universe extends c/H0 ~ 3000h-1Mpc, most observational works to map the distribution of galaxies so far have been mainly applied to samples within ~ 100h-1Mpc from us. Thus a CfA redshift survey slice, for example, of 8h < α < 17h, 26.5° < δ < 32.5°, and cz ≾ 15000km/sec (de Lapparent et al. 1986, 1988) represents merely ~ 2 x 10-5 of the total volume of the observable universe. This clearly illustrates the importance of examining possible systematic biases and variations in the estimates of two-point correlation functions from instrinsically limited data. We studied such sample-to-sample variations by analysing subsamples extracted from large N-body simulation data.

scholarly journals The 2dF QSO Redshift Survey - XIV. Structure and evolution from the two-point correlation function

2005 ◽  
Vol 356 (2) ◽  
pp. 415-438 ◽  
Author(s):  
Scott M. Croom ◽  
B. J. Boyle ◽  
T. Shanks ◽  
R. J. Smith ◽  
L. Miller ◽  
...  
Keyword(s):  
Correlation Function ◽  
Point Correlation ◽  
Point Correlation Function ◽  
Redshift Survey

Power spectrum, correlation function, and tests for luminosity bias in the CfA redshift survey

1994 ◽  
Vol 431 ◽  
pp. 569 ◽  
Author(s):  
Changbom Park ◽  
Michael S. Vogeley ◽  
Margaret J. Geller ◽  
John P. Huchra
Keyword(s):  
Correlation Function ◽  
Power Spectrum ◽  
Redshift Survey ◽  
Spectrum Correlation

scholarly journals Anisotropic extinction distortion of the galaxy correlation function

2011 ◽  
Vol 84 (6) ◽  
Author(s):  
Wenjuan Fang ◽  
Lam Hui ◽  
Brice Ménard ◽  
Morgan May ◽  
Ryan Scranton
Keyword(s):  
Correlation Function ◽  
The Galaxy

scholarly journals The galaxy correlation function as a constraint on galaxy formation physics

2016 ◽  
Vol 458 (1) ◽  
pp. 934-949 ◽  
Author(s):  
Marcel P. van Daalen ◽  
Bruno M. B. Henriques ◽  
Raul E. Angulo ◽  
Simon D. M. White
Keyword(s):  
Correlation Function ◽  
Galaxy Formation ◽  
The Galaxy
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