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

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dc.creatorRigopoulou, D.
dc.creatorFranceschini, A.
dc.creatorGenzel, R.
dc.creatorvan der Werf, P.
dc.creatorAussel, H.
dc.creatorCesarsky, C.
dc.creatorDennefeld, M.
dc.creatorOliver, S.
dc.creatorRowan-Robinson, M.
dc.date1999-12-29
dc.date2000-01-11
dc.date.accessioned2026-07-07T02:35:14Z
dc.date.available2026-07-07T02:35:14Z
dc.descriptionA 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.
dc.description8 pages, 3 figures, to appear in "ISO Surveys of a Dusty Universe", eds. D. Lemke, M. Stickel, K. Wilke, typos corrected
dc.identifierhttps://arxiv.org/abs/astro-ph/9912544
dc.identifierhttp://arxiv.org/abs/astro-ph/9912544
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15540
dc.subjectAstrophysics
dc.titleNIR Spectroscopy with the VLT of a sample of ISO selected Hubble Deep Field South Galaxies
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