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S. Heinis, B. Milliard, S. Arnouts (Laboratoire d'Astrophysique de Marseille), D. Schiminovich (Columbia University), O. Ilbert (Laboratoire d'Astrophysique de Marseille), T. Budavari (John Hopkins University), J. Blaizot, B. Meneux (Laboratoire d'Astrophysique de Marseille), GALEX Science Team
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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Bulletin of the American Astronomical Society, 36 5
© 2004. The American Astronomical Society.