The Small-Scale Angular Correlation Function for a High-Galactic Latitude Faint Field

Details The Small-Scale Angular Correlation Function for a High-Galactic Latitude Faint Field The Small-Scale Angular Correlation Function for a High-Galactic Latitude Faint Field

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aas...182.3001w&link_type=abstract

American Astronomical Society, 182nd AAS Meeting, #30.01; Bulletin of the American Astronomical Society, Vol. 25, p.836

Astronomy and Astrophysics

Astronomy

Scientific paper

The galaxies in a high-galactic latitude field are analysed for clustering using angular correlation analysis. Our sample is unique in that, with a total of 10h of exposure time in V, R and I distributed equally between filters, the seeing for the summed frames is ~ 0.7 arcsec. Data of this quality allows us to measure the galaxy correlation function to very small angular separations. A preliminary analysis of the ellipticity distribution of the observed galaxies is also presented.

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