Publication Date

2008

Comments

This 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-y

Abstract

I 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.

Pages

977-983

Volume

112

Issue

9-11

Journal Title

Nuovo Cimento B