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astro-ph.CO2012★ 33 cited
Comparison of star formation rates from Halpha and infrared luminosities as seen by Herschel
H. Domínguez, M. Mignoli, F. Pozzi +55
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 conversio…
astro-ph.CO2012★ 3 cited
Fast radiative transfer of dust reprocessing in semi-analytic models with artificial neural networks
Laura Silva, Fabio Fontanot, Gian Luigi Granato
A serious concern for semi-analytical galaxy formation models, aiming to simulate multi-wavelength surveys and to thoroughly explore the model parameter space, is the extremely tim…