The TNG EROs Spectroscopic Identification Survey (TESIS)

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dc.creatorSaracco, P.
dc.creatorLonghetti, M.
dc.creatorDella Ceca, R.
dc.creatorSevergnini, P.
dc.creatorBraito, V.
dc.creatorBender, R.
dc.creatorDrory, N.
dc.creatorFeulner, G.
dc.creatorHopp, U.
dc.creatorMannucci, F.
dc.creatorMaraston, C.
dc.date2003-09-10
dc.date.accessioned2026-07-07T02:09:31Z
dc.date.available2026-07-07T02:09:31Z
dc.descriptionWe are carrying on a near-IR very low resolution spectroscopic follow-up in parallel with XMM-Newton observations of a complete sample of ~30 bright (K'<18.5) Extremely Red Objects (EROs) selected over an area of 360 arcmin^2 of the MUNICS survey. We here present the preliminary results of the spectroscopic and X-ray data analysis.
dc.description2 pages, "Multiwavelength Cosmology" Mykonos, June 2003, conference proceedings
dc.identifierhttps://arxiv.org/abs/astro-ph/0309289
dc.identifierhttp://arxiv.org/abs/astro-ph/0309289
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6458
dc.subjectAstrophysics
dc.titleThe TNG EROs Spectroscopic Identification Survey (TESIS)
dc.typetext

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