Clustering Evolution of Star-Forming Galaxies from the VVDS/GALEX Survey

Details Clustering Evolution of Star-Forming Galaxies from the VVDS/GALEX Survey Clustering Evolution of Star-Forming Galaxies from the VVDS/GALEX Survey

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..379..318m&link_type=abstract

Cosmic Frontiers ASP Conference Series, Vol. 379, proceedings of the conference held 31 July-4 August 2006 at Durham University,

Physics

Scientific paper

We present in this poster the clustering properties of different type of galaxies selected in optical and ultraviolet in the VVDS-02h field from the VVDS/GALEX survey. When selected in optical, we observe that early-type galaxies have a higher clustering amplitude than late-type ones up to z˜1.2. In NUV and FUV, we observe a subsample of the optically selected late-type galaxies which are brighter, with higher stellar masses and more active on average. The clustering amplitude of these UV selected star-forming galaxies is higher.

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