TESIS - The TNG EROs Spectroscopic Identification Survey

Details TESIS - The TNG EROs Spectroscopic Identification Survey TESIS - The TNG EROs Spectroscopic Identification Survey

2002-07-17

arxiv.org/abs/astro-ph/0207352v1

Astronomy and Astrophysics

Astrophysics

For the proceedings of the meeting "Galaxy Evolution: Theory and Observations", (Cozumel, April 2002), to be edited by V. Avil

Scientific paper

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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