Population synthesis modelling of luminous infrared galaxies at intermediate redshift

Details Population synthesis modelling of luminous infrared galaxies at intermediate redshift Population synthesis modelling of luminous infrared galaxies at intermediate redshift

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010sf2a.conf...41g&link_type=abstract

SF2A-2010: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics. Eds.: S. Boissier, M. Heydari-

Astronomy and Astrophysics

Astrophysics

Galaxies Evolution, Infrared, Bayesian Analysis, Stellar Content, Sed-Fitting

Scientific paper

Luminous InfraRed Galaxies (LIRGs) are particularly important for studying the {build-up} of the stellar mass from z=1 to z=0, and for determining physical properties of these objects at redshift 0.7. The global star formation rate (SFR) at z ˜ 0.7 is mainly produced by LIRGs.We perform a multiwavelength study of an LIRGs sample in the Extended Chandra Deep Field South at z=0.7, selected at 24 μm by MIPS onboard Spitzer Space Telescope and detected in 17 filters. Data go from the near-ultraviolet to the mid-infrared. We distinguish a subsample of galaxies detected at 70 μ m, which we compare to the rest of the sample to investigate the relative importance of this wavelength in determining of the physical parameters.

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