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

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

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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D. Rigopoulou, A. Franceschini, R. Genzel, P. van der Werf, H. Aussel, C. Cesarsky, M. Dennefeld, S. Oliver, M. Rowan-Robinson. 2000-01-11. NIR Spectroscopy with the VLT of a sample of ISO selected Hubble Deep Field South Galaxies. https://arxiv.org/abs/astro-ph/9912544

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