NIR Spectroscopy with the VLT of a sample of ISO selected Hubble Deep Field South Galaxies

Details NIR Spectroscopy with the VLT of a sample of ISO selected Hubble Deep Field South Galaxies NIR Spectroscopy with the VLT of a sample of ISO selected Hubble Deep Field South Galaxies

1999-12-29

arxiv.org/abs/astro-ph/9912544v2

Astronomy and Astrophysics

Astrophysics

8 pages, 3 figures, to appear in "ISO Surveys of a Dusty Universe", eds. D. Lemke, M. Stickel, K. Wilke, typos corrected

Scientific paper

A new population of faint galaxies characterized by an extremely high rate of evolution with redshift up to z~1.5 has recently been discovered by ISO. These sources are likely to contribute significantly to the cosmic far-IR extragalactic background. We have carried out near-infrared VLT-ISAAC spectroscopy of a sample of ISOCAM galaxies from the Hubble Deep Field South. The rest-frame R-band spectral properties of the ISO population resembles that of powerful dust-enshrouded active starburst galaxies.

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