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27 April 2024
 
  » arxiv » astro-ph/0505101

 Article overview



Spitzer view on the evolution of star-forming galaxies from z=0 to z~3
Pablo G. Perez-Gonzalez ; George H. Rieke ; Eiichi Egami ; Almudena Alonso-Herrero ; Herve Dole ; Casey Papovich ; Myra Blaylock ; Jessica Jones ; Marcia Rieke ; Jane Rigby ; Pauline Barmby ; Giovanni G. Fazio ; Jiasheng Huang ; Christopher Martin ;
Date 5 May 2005
Journal Astrophys.J. 630 (2005) 82-107
Subject astro-ph
Affiliation2,1), Herve Dole (3,1), Casey Papovich , Myra Blaylock , Jessica Jones , Marcia Rieke , Jane Rigby , Pauline Barmby , Giovanni G. Fazio , Jiasheng Huang , Christopher Martin ( Steward Observatory, University of Arizona, USA; Instituto de Estructura
AbstractWe use a 24 micron selected sample containing more than 8,000 sources to study the evolution of star-forming galaxies in the redshift range from z=0 to z~3. We obtain photometric redshifts for most of the sources in our survey using a method based on empirically-built templates spanning from ultraviolet to mid-infrared wavelengths. The accuracy of these redshifts is better than 10% for 80% of the sample. The derived redshift distribution of the sources detected by our survey peaks at around z=0.6-1.0 (the location of the peak being affected by cosmic variance), and decays monotonically from z~1 to z~3. We have fitted infrared luminosity functions in several redshift bins in the range 01.e11 L_sun) to the total SFR density increases steadily from z~0 up to z~2.5, forming at least half of the newly-born stars by z~1.5. Ultraluminous infrared galaxies (L_TIR>1.e12 L_sun) play a rapidly increasing role for z>~1.3.
Source arXiv, astro-ph/0505101
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