TESIS - The TNG EROs Spectroscopic Identification Survey

P. Saracco; M. Longhetti; P. Severgnini; R. Della Ceca; R. Bender; N. Drory; G. Feulner; F. Ghinassi; U. Hopp; F. Mannucci; C. Maraston

arXiv · astro-ph/0207352

TESIS - The TNG EROs Spectroscopic Identification Survey

P. Saracco·M. Longhetti·P. Severgnini·R. Della Ceca·R. Bender·N. Drory·G. Feulner·F. Ghinassi·U. Hopp·F. Mannucci·C. Maraston

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Abstract

A near-IR low-resolution spectroscopic follow-up of a complete sample of K<18.5 EROs has started at the 3.5 m Telescopio Nazionale Galileo (TNG, La Palma, Canary Islands) by using a prism disperser AMICI. The sample has been selected from the Munich Near-IR Cluster Survey (MUNICS). The project aims at revealing massive galaxies at z>1.2 and at estimating their spatial density to put constraints on the galaxy formation and evolution models. In this proceeding, the preliminary analysis of the first spectra obtained is presented.

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P. Saracco, M. Longhetti, P. Severgnini, R. Della Ceca, R. Bender, N. Drory, G. Feulner, F. Ghinassi, U. Hopp, F. Mannucci, C. Maraston. 2002-07-17. TESIS - The TNG EROs Spectroscopic Identification Survey. https://arxiv.org/abs/astro-ph/0207352

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