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Shards of SHARDS: emission line galaxies

Published online by Cambridge University Press:  21 March 2013

Antonio Cava
Affiliation:
Departamento de Astrofísica, Facultad de CC. Físicas, Universidad Complutense de Madrid, E-28040 Madrid, Spain, email: acava@fis.ucm.es
Víctor Villar
Affiliation:
Departamento de Astrofísica, Facultad de CC. Físicas, Universidad Complutense de Madrid, E-28040 Madrid, Spain, email: acava@fis.ucm.es
Pablo G. Pérez-González
Affiliation:
Departamento de Astrofísica, Facultad de CC. Físicas, Universidad Complutense de Madrid, E-28040 Madrid, Spain, email: acava@fis.ucm.es 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
Corresponding
E-mail address:
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Abstract

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.

Type
Contributed Papers
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

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