The clustering of rest-UV selected galaxies from GALEX deep fields

Details The clustering of rest-UV selected galaxies from GALEX deep fields The clustering of rest-UV selected galaxies from GALEX deep fields

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...205.2503h&link_type=abstract

American Astronomical Society Meeting 205, #25.03; Bulletin of the American Astronomical Society, Vol. 36, p.1384

Astronomy and Astrophysics

Astronomy

Scientific paper

The status and preliminary results for the Angular Correlation Function (ACF) of rest-UV selected galaxies in GALEX deep fields are presented. This first determination of the ACF of UV-selected galaxies at z 1 rests on more than 5,000 galaxies brighter than NUV AB magnitude 24, in a 0.5 degree radius area. The slope of the ACF is found similar to that observed for star-forming galaxies selected at visible wavelengths in the local Universe, and for LBGs at z 3. We discuss the evolution of the bias of the rest-UV selected galaxies between z 0 and z 3. GALEX is a NASA SMEX mission developped in collaboration with France and Korea.

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