AAS 207th Meeting, 8-12 January 2006
Session 69 Stellar Evolution
Poster, Tuesday, 9:20am-6:30pm, January 10, 2006, Exhibit Hall

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[69.07] VVDS-SWIRE evolution of the rest frame K-band luminosity function from z=1.5

S. Arnouts (Laboratoire d'Astrophysique de Marseille), C.J. Lonsdale (IPAC, Caltech), O. Ilbert (Bologna Observatory), M. Rowan-Robinson (Imperial College), O. Le Fevre (Laboratoire d'Astrophysique de Marseille), S.J. Oliver (University of Sussex), V. Le Brun (Laboratoire d'Astrophysique de Marseille), M.C. Polletta (University of California, San Diego), VVDS Collaboration, SWIRE Team

The evolution of the rest frame K-band luminosity function is computed over the redshift range 0 to z=1.5 from 3780 measured redshifts of SWIRE 3.6microns-selected sources brighter than 5 microJy. We explore the evolution of the older stellar populations accross cosmic time.

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