Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-01-10
Astronomy and Astrophysics
Astrophysics
To be published in "Starburst Galaxies Near and Far", eds. D. Lutz and L. Tacconi, Springer
Scientific paper
This is a summary of arguments in favor of observing high-redshift star formation in the UV as presented at the Ringberg meeting in September 2000. The most rapidly star-forming galaxies are very dusty, easier to detect at 850um than in the UV, but less rapidly star-forming galaxies are less obscured by dust and as a result the comparatively faint galaxies that hosted most high-redshift star formation are easiest to detect in the UV. The correlation of star-formation rate and dust obscuration implies that extremely luminous dusty galaxies are usually as bright in the UV as the less luminous dust-free galaxies, and that any UV survey at a given redshift 0
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