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Shards of SHARDS: emission line galaxies

Published online by Cambridge University Press:  21 March 2013

Antonio Cava ,
Víctor Villar ,
Pablo G. Pérez-González  and
the SHARDS Team
Antonio Cava
Affiliation:
Departamento de Astrofísica, Facultad de CC. Físicas, Universidad Complutense de Madrid, E-28040 Madrid, Spain, email: [email protected]
Víctor Villar
Affiliation:
Departamento de Astrofísica, Facultad de CC. Físicas, Universidad Complutense de Madrid, E-28040 Madrid, Spain, email: [email protected]
Pablo G. Pérez-González
Affiliation:
Departamento de Astrofísica, Facultad de CC. Físicas, Universidad Complutense de Madrid, E-28040 Madrid, Spain, email: [email protected] Associate Astronomer at Steward Observatory, The University of Arizona
the SHARDS Team
Affiliation:
SHARDS Team webpage: http://guaix.fis.ucm.es/~pgperez/SHARDS/team.html
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Abstract

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SHARDS (Survey for High-z Absorption Red & Dead Sources; see Pérez-González et al. 2012) is an optical ultra-deep spectro-photometric survey with OSIRIS-GTC aimed at selecting and studying massive passively evolving galaxies at z=1.0–2.3 in GOODS-North. Nonetheless, the data quality allow a plethora of studies on galaxy populations, including Emission Line Galaxies (ELGs) about which we have started our first science verification project. The selection procedure, measurement and first analysis of ELGs in SHARDS, demonstrate the huge capability of the survey in providing physical information for a large sample of emitters, spanning from local Hα to high-z Lyman-α emitters.

Keywords

galaxies: high-redshift — galaxies: fundamental parameters — galaxies: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S292: Molecular Gas, Dust, and Star Formation in Galaxies , August 2012 , pp. 189
Copyright
Copyright © International Astronomical Union 2013

References

Cava, A. & Pérez González, P. G., the SHARDS Team 2012, arXiv:1201.2177Google Scholar
Pérez-González, P. G., Cava, A., Barro, G., et al. 2012, ApJ accepted, arXiv:1207.6639Google Scholar