Results from a Sample of 1000 Field Galaxies

  • Edwin D. Loh
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 141)


The angular correlation function for galaxies with redshifts z between 0.15 and 0.85 has been measured. The data are fitted to a spatial correlation function of the form ξ(rp) = (r 0/ rp)γ(1+ z)-(3+∊), where r p is the proper distance, and is a measure of the evolution of the clustering. These data and other local measurements imply r 0 = (4.8 t 0.3)h -1 Mpc and = -0.5 ± 0.5 for an Einstein-deSitter universe (Ω = 1). If instead Ω = 0, then = -1.3 ± 0.5; i. e., clustering was stronger in the past. Thus the data are consistent with the assumptions that Ω = 1 and that physical associations of galaxies neither expand nor contract ( = 0).


Correlation Function Spatial Correlation Function Virgo Cluster Photometric Redshift Angular Correlation Function 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


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Copyright information

© Kluwer Academic Publishers 1988

Authors and Affiliations

  • Edwin D. Loh
    • 1
  1. 1.Joseph Henry LaboratoriesPrinceton UniversityPrincetonUSA

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