Galaxy evolution studies observing Emission Line Galaxies with the GTC

Bibcode
2003RMxAC..16..221G
Gallego, J.
Bibliographical reference

Science with the GTC (Eds. José Miguel Rodríguez Espinosa, Francisco Garzón López, and Verónica Melo Martín) Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) Vol. 16, pp. 221-224 (2003) (http://www.astroscu.unam.mx/~rmaa/)

Advertised on:
0
2003
Number of authors
1
IAC number of authors
0
Citations
0
Refereed citations
0
Description
Emission line galaxies are the most easily detected and studied objects in the high redshift Universe. They are being used to trace the evolution of the critical observables of the Universe such as star formation rate densities, starburst properties, and abundances. The GTC will be a very powerful tool for studying the evolution of emission line galaxy populations at different redshifts. Large surveys, such as OTELO, carried out with OSIRIS and extended by follow-up spectroscopic studies in the near infrared using EMIR will enable the GTC to make a major impact in extragalactic astronomy.
Type
Non-refereed
Galaxies

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