Publication Date

2007

Journal or Book Title

NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-GENERAL PHYSICS RELATIVITY ASTRONOMY AND MATHEMATICAL PHYSICS AND METHODS

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.

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

Pages

971-976

Volume

122

Issue

9-11

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