Galaxy clustering at B ≡ 25m.

Details Galaxy clustering at B ≡ 25m. Galaxy clustering at B ≡ 25m.

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993wfinw...3....7r&link_type=abstract

IAU Working Group on Wide-Field Imaging, Newsl., No. 3, p. 7 - 9

Physics

Galaxy Clustering, Galaxies: Redshifts

Scientific paper

The authors find the angular two-point correlation function,
ω(θ), amplitude for faint galaxies to be significantly
lower than would be expected for a model in which clustering is stable
in proper co-ordinates and the redshift distribution maintains a
no-evolution form.

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