The 10^{11} M_{&sun;} Question: Massive Galaxies at z_{phot} < 2 and the Rise of the Red Sequence

Details The 10^{11} M_{&sun;} Question: Massive Galaxies at z_{phot} < 2 and the Rise of the Red Sequence The 10^{11} M_{&sun;} Question: Massive Galaxies at z_{phot} < 2 and the Rise of the Red Sequence

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..399..173t&link_type=abstract

Panoramic Views of Galaxy Formation and Evolution ASP Conference Series, Vol. 399, proceedings of the conference held 11-16 Dece

Astronomy and Astrophysics

Astronomy

Scientific paper

I present and analyse the color--stellar mass diagram for z_phot < 2 galaxies, using a K-selected catalogue of the Extended Chandra Deep Field South (ECDFS) from the MUltiwavelength Survey by Yale--Chile (MUSYC). The results suggest a long, slow migration of massive galaxies onto the red sequence, occuring over many Gyr: at most 1/5 of all massive galaxies were already on the red sequence at z ˜ 2, and at least 1/2 have only re(joined) the red sequence since z ˜ 1.

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