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

A. Franceschini; C. Cesarsky; D. Rigopoulou; H. Aussel; M. Dennefeld; M. Rowan-Robinson; P. van der Werf; R. Genzel; S. Oliver

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

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arxiv astro-ph/9912544 v2 pith:H7WBCHL3 submitted 1999-12-29 astro-ph

D. Rigopoulou , A. Franceschini , R. Genzel , P. van der Werf , H. Aussel , C. Cesarsky , M. Dennefeld , S. Oliver

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M. Rowan-Robinson

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keywords galaxiesdeepfieldhubblepopulationsamplesouthspectroscopy

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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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