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A consistent view on star-forming galaxies at high redshift from multi-wavelength observations and SED modeling

Published online by Cambridge University Press:  17 August 2016

Daniel Schaerer ,
Stephane de Barros  and
Frederic Boone
Daniel Schaerer
Affiliation:
Observatoire de Genève, Université de Genève, 51 Ch. des Maillettes, 1290 Versoix, Switzerland email: [email protected] CNRS, IRAP, 14 Avenue E. Belin, 31400 Toulouse, France
Stephane de Barros
Affiliation:
INAF-Osservatorio Astronomico di Bologna, via Ranzani 1, 40127, Bologna, Italy
Frederic Boone
Affiliation:
CNRS, IRAP, 14 Avenue E. Belin, 31400 Toulouse, France
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Abstract

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We stress the importance of consistent SED analysis for distant star-forming galaxies (SFGs). We then summarise recent results from such an analysis concerning their basic physical properties, such as the determination of star formation rate (SFR), stellar mass, specific star SFR, UV attenuation, and how this affects our knowledge of star formation properties at high-z.

Keywords

Galaxies: starburstGalaxies: high-redshift
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S319: Galaxies at High Redshift and Their Evolution Over Cosmic Time , August 2015 , pp. 45 - 48
Copyright
Copyright © International Astronomical Union 2016 

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