The EROs at z < 1.5 in the Groth-Westphal field of the GOYA survey

Bibcode
2005RMxAC..24..270P
Prieto, M.; Balcells, M.; Domínguez-Palmero, L.; Cristóbal-Hornillos, D.; Erwin, P.; Eliche-Moral, C.; Abreu, D.
Bibliographical reference

II International GTC Workshop: Science with GTC 1st-light Instruments and the LMT (Eds. A. M. Hidalgo-Gámez, J. J. González, J. M. Rodríguez Espinosa, and S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) Vol. 24, pp. 270-270 (2005) (http://www.astroscu.unam.mx/~rmaa/)

Advertised on:
12
2005
Number of authors
7
IAC number of authors
0
Citations
1
Refereed citations
1
Description
The study of the Extremly Red Objects (EROs), is the importance for setting constraints on the first epoch of massive galaxy formation, for exploring the population of dust reddened starburst and for testing models of galaxy formation in general. They are defined as objects with I-K>4(Vega). The traditional picture identifies the EROs either with passively evolving elliptical galaxies, or with young starburst reddened dust.
Type
Non-refereed
Galaxies
Star formation

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