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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
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Abstract

We 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 0 1.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.

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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. 2005-05-05. Spitzer view on the evolution of star-forming galaxies from z=0 to z~3. https://doi.org/10.1086/431894

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