Science-advisor
REGISTER info/FAQ
Login
username
password
     
forgot password?
register here
 
Research articles
  search articles
  reviews guidelines
  reviews
  articles index
My Pages
my alerts
  my messages
  my reviews
  my favorites
 
 
Stat
Members: 3645
Articles: 2'506'133
Articles rated: 2609

26 April 2024
 
  » arxiv » astro-ph/9608001

 Article overview



The two-point correlation function and morphological segregation in the Optical Redshift Survey
Sune Hermit ; Basilio X. Santiago ; Ofer Lahav ; Michael A. Strauss ; Marc Davis ; Alan Dressler ; John P. Huchra ;
Date 1 Aug 1996
Subject astro-ph
AffiliationAstronomical Observatory, Copenhagen), Basilio X. Santiago (Institute of Astronomy, Cambridge UK), Ofer Lahav (Institute of Astronomy, Cambridge UK), Michael A. Strauss (Dept. of Astrophysical Sciences, Princeton), Marc Davis (Physics and Astronomy Dep
AbstractWe study the clustering of galaxies in real and redshift space using the Optical Redshift Survey (ORS). We estimate the two point correlation function in redshift space, $xi(s)$, for several subsamples of ORS, spanning nearly a factor of 30 in volume and detect significant variations in $xi(s)$ among the subsamples covering small volumes. For volumes gtsima $(75 h^{-1} { m Mpc})^{3}$ the ORS subsamples present very similar clustering patterns. Powerlaw fits to $xi(s)$ give best-fit values in the range $1.5 leq gamma_{s} leq 1.7 $ and $6.5 leq s_{0} leq 8.8 h^{-1}$ Mpc for several samples extending to redshifts of 8000 km s$^{-1}$. We find that $xi(s)$ is larger for the magnitude-limited sample than for diameter-limited one within a radius of 4000 km s$^{-1}$. We interpret this as an indirect result of morphological segregation coupled with differences in morphological mix. We split ORS into morphological subsamples and confirm the existence of morphological segregation of galaxies out to scales of $s sim 10 h^{-1}$ Mpc. Our results indicate that the relative bias factor between early type galaxies and late-types may be weakly dependent on scale. If real, this would suggest non-linear biasing. We also compute correlations as a function of radial and projected separations, $xi(r_p, pi)$ and derive the real space correlation function, $xi(r)$. The results obtained in real space confirm those found using $xi(s)$.
Source arXiv, astro-ph/9608001
Services Forum | Review | PDF | Favorites   
 
Visitor rating: did you like this article? no 1   2   3   4   5   yes

No review found.
 Did you like this article?

This article or document is ...
important:
of broad interest:
readable:
new:
correct:
Global appreciation:

  Note: answers to reviews or questions about the article must be posted in the forum section.
Authors are not allowed to review their own article. They can use the forum section.

browser Mozilla/5.0 AppleWebKit/537.36 (KHTML, like Gecko; compatible; ClaudeBot/1.0; +claudebot@anthropic.com)






ScienXe.org
» my Online CV
» Free


News, job offers and information for researchers and scientists:
home  |  contact  |  terms of use  |  sitemap
Copyright © 2005-2024 - Scimetrica