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28 April 2024
 
  » arxiv » astro-ph/9608142

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A wide-field K-band survey - II. Galaxy clustering
C.M. Baugh ; J.P.Gardner ; C.S. Frenk ; R.M. Sharples ;
Date 22 Aug 1996
Subject astro-ph
AffiliationUniversity of Durham
AbstractWe present the first measurement of the angular correlation function in a $K$-selected galaxy survey, from two fields covering almost 10 square degrees. The angular correlation function at small angles is well described by a $ heta^{-0.8}$ power law, as for optically selected samples. The clustering amplitude is reduced by a factor of $sim 4$ between galaxies with $K<15$ and a fainter magnitude slice with $15
Source arXiv, astro-ph/9608142
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