A "UV+IR" history of star formation at 0<z<1

Details A "UV+IR" history of star formation at 0<z<1 A "UV+IR" history of star formation at 0<z<1

2005-06-20

arxiv.org/abs/astro-ph/0506463v1

Astronomy and Astrophysics

Astrophysics

5 pages, to appear in the proceedings of the conference "Rencontres de Moriond" held in La Thuile, Italy (March 6-12th, 2005),

Scientific paper

The combination of both contributions from the observed UV emission and the absorbed radiations reprocessed in the infrared represents the ideal approach to constrain the activity of massive star formation in galaxies. Using recent results from GALEX and Spitzer, we compare the evolutions of the UV and IR energy densities with redshift as well as their contributions to the star formation history at 0 10^11 L_sol).

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