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 dustenshrouded active starburst galaxies.
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Rigopoulou, D. et al. (2000). NIR Spectroscopy with the VLT of a Sample of ISO Selected Hubble Deep Field South Galaxies. In: Lemke, D., Stickel, M., Wilke, K. (eds) ISO Surveys of a Dusty Universe. Lecture Notes in Physics, vol 548. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-45553-1_31
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DOI: https://doi.org/10.1007/3-540-45553-1_31
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