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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
; | Date: |
5 May 2005 | Journal: | Astrophys.J. 630 (2005) 82-107 | Subject: | astro-ph | Affiliation: | 2,1), 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 | 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 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 | Services: | Forum | Review | PDF | Favorites |
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