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Caputi, K. Kovac, L. A. M. Tasca, L. de Ravel, L. Pozzetti, L. Riguccini, L. Silva, L. Tresse, M. Bolzonella, M. Mignoli, M. S\\'anchez-Portal, M. Scodeggio, M. Tanaka, O. Cucciati, O. LeFevr\\`e, P. Franzetti, P. Kampczyk, P. Nair, R. Maiolino, R. Nordon, R. Pell\\`o, S. Bardelli, S. Berta, S. de la Torre, S. J. Lilly, S. Wuyts, T. Contini, V. le Brun. C. Maier, V. Mainieri, Y. Peng","submitted_at":"2012-05-21T11:59:02Z","abstract_excerpt":"We empirically test the relation between the SFR(LIR) derived from the infrared luminosity, LIR, and the SFR(Ha) derived from the Ha emission line luminosity using simple conversion relations. We use a sample of 474 galaxies at z = 0.06 - 0.46 with both Ha detection (from 20k zCOSMOS survey) and new far-IR Herschel data (100 and 160 {\\mu}m). We derive SFR(Ha) from the Ha extinction corrected emission line luminosity. We find a very clear trend between E(B - V) and LIR that allows to estimate extinction values for each galaxy even if the Ha emission line measurement is not reliable. 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Bongiorno, A. Cimatti, A. Iovino, A. Renzini, B. Garilli, B. Magnelli, C. Gruppioni, C. Knobel, C. M. Carollo, D. Elbaz, D. Lutz, D. Vergani, E. LeFloc'h, E. P\\'erez-Montero, E. Riccardelli, E. Zucca, F. Calura, F. Lamareille, F. Mateucci, F. Pozzi, G. Coppa, G. L. Granato, G. Zamorani, H. Dom\\'inguez, J. Cepa, J.-F. Le Borgne, J.-P. Kneib, J. Silverman, K. Caputi, K. Kovac, L. A. M. Tasca, L. de Ravel, L. Pozzetti, L. Riguccini, L. Silva, L. Tresse, M. Bolzonella, M. Mignoli, M. S\\'anchez-Portal, M. Scodeggio, M. Tanaka, O. Cucciati, O. LeFevr\\`e, P. Franzetti, P. Kampczyk, P. Nair, R. Maiolino, R. Nordon, R. Pell\\`o, S. Bardelli, S. Berta, S. de la Torre, S. J. Lilly, S. Wuyts, T. Contini, V. le Brun. C. Maier, V. Mainieri, Y. 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