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Star formation properties of UV selected galaxies in the ELAIS field

Published online by Cambridge University Press:  01 December 2006

J. Iglesias-Páramo ,
V. Buat ,
J. Hernández-Fernández ,
C. K. Xu  and
D. Burgarella
J. Iglesias-Páramo
Affiliation:
Instituto de Astrofísica de Andalucía (C.S.I.C.), SPAIN emails: [email protected], [email protected]
V. Buat
Affiliation:
Observatoire Astronomique de Marseille Provence, FRANCE emails: [email protected], [email protected]
J. Hernández-Fernández
Affiliation:
Instituto de Astrofísica de Andalucía (C.S.I.C.), SPAIN emails: [email protected], [email protected]
C. K. Xu
Affiliation:
California Institute of Technology, Pasadena, USA email: [email protected]
D. Burgarella
Affiliation:
Observatoire Astronomique de Marseille Provence, FRANCE emails: [email protected], [email protected]
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Abstract

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Properties related to dust attenuation and star formation of an UV selected sample of intermediate redshift galaxies are presented in this work. We find hints of a decrease of the LIR/LFUV ratio with increasing redshift at low values of the total luminosity. Downsizing is observed at all redshifts, and the SSFR is found to increase with increasing redshift at all stellar masses.

Keywords

galaxies: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S241: Stellar Populations as Building Blocks of Galaxies , December 2006 , pp. 567 - 568
Copyright
Copyright © International Astronomical Union 2007

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