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/Università di Bologna
2 OABO - INAF - Osservatorio Astronomico di Bologna
3 Unipd - Università degli Studi di Padova = University of Padua
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

Aims. In this paper we use a well-controlled spectroscopic sample of galaxies at 1 

Keywords: galaxies: high-redshift; galaxies: star formation; ultraviolet: galaxies; infrared: galaxies; techniques: spectroscopic

Domains: Physics [physics]; Astrophysics [astro-ph]

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, 2015, 582, pp.A80. ⟨10.1051/0004-6361/201425430⟩. ⟨cea-01383747⟩