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The star formation rate cookbook at 1 < z < 3: Extinction-corrected relations for UV and [OII]λ3727 luminosities

M. Talia 1, 2 Alessandro Cimatti 1 L. Pozzetti 2 G. Rodighiero 3 C. Gruppioni 2 F. Pozzi 1 Emanuele Daddi 4 C. Maraston 5 M. Mignoli 2 J. Kurk 6
1 University of Bologna
2 OABO - INAF - Osservatorio Astronomico di Bologna
3 Universita degli Studi di Padova
4 DAP - Département d'Astrophysique (ex SAP)
5 Institute of Cosmology and Gravitation - Institute of Cosmology and Gravitation
6 MPE - Max-Planck-Institut für Extraterrestrische Physik
Abstract : Aims. In this paper we use a well-controlled spectroscopic sample of galaxies at 1 
Keywords : infrared: galaxies techniques: spectroscopic galaxies: high-redshift galaxies: star formation ultraviolet: galaxies
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CEA | DSM-IRFU | IRFU-SAP | UNIV-PARIS-SACLAY | CEA-UPSAY | CEA-DRF

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M. Talia, Alessandro Cimatti, L. Pozzetti, G. Rodighiero, C. Gruppioni, et al.. The star formation rate cookbook at 1 < z < 3: Extinction-corrected relations for UV and [OII]λ3727 luminosities. Astronomy and Astrophysics - A&A, EDP Sciences, 2015, 582, pp.A80. ⟨10.1051/0004-6361/201425430⟩. ⟨cea-01383747⟩

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