2005ApJ...630...82P

We use a 24 µm-selected sample containing more than 8000 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<z≲3. Our results constrain the density and/or luminosity evolution of infrared-bright star-forming galaxies. The typical infrared luminosity (L^*) decreases by an order of magnitude from z∼2 to the present. The cosmic star formation rate (SFR) density goes as (1+z)^4.0±0.2 from z=0 to 0.8. From z=0.8 to z∼1.2, the SFR density continues rising with a smaller slope. At 1.2<z≲3, the cosmic SFR density remains roughly constant. The SFR density is dominated at low redshift (z≲0.5) by galaxies that are not very luminous in the infrared (L_TIR<10¹¹ L_☉, where L_TIRis the total infrared luminosity, integrated from 8 to 1000 µm). The contribution from luminous and ultraluminous infrared galaxies (L_TIR>10¹¹ L_☉) 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>10¹² L_☉) play a rapidly increasing role for z≳1.3.