A wide-field K-band survey - II. Galaxy clustering

Details A wide-field K-band survey - II. Galaxy clustering A wide-field K-band survey - II. Galaxy clustering

1996-08-22

arxiv.org/abs/astro-ph/9608142v1

Astronomy and Astrophysics

Astrophysics

5 pages, 4 postscript figures included. Uses mn.sty. To be published as a Letter in Monthly Notices of the RAS. Postscript ver

Scientific paper

We 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 $\theta^{-0.8}$ 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

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