Calzetti, D2024-04-262024-04-262008-01-01https://doi.org/10.1393/ncb/i2008-10432-yhttps://hdl.handle.net/20.500.14394/3521This is the pre-published version harvested from ArXiv. The published version is located at http://paperseek.sif.it/index.php?doi=10.1393/ncb/i2008-10432-yI review measurements of star formation in nearby galaxies in the UV-to-FIR wavelength range, and discuss their impact on SFR determinations in intermediate and high redshift galaxy populations. Existing and upcoming facilities will enable precise cross-calibrations among the various indicators, thus bringing them onto a common scale.Astrophysics and Astronomyarticle