Stellar masses of star-forming galaxies at 0.3 < z < 1.2 in the GOYA survey

Bibcode
2005RMxAC..24..227C
Cristóbal-Hornillos, D.; Balcells, M.; Domínguez-Palmero, L.; Eliche-Moral, C.; Erwin, P.; Guzmán, R.; Prieto, M.
Referencia bibliográfica

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. 227-228 (2005) (http://www.astroscu.unam.mx/~rmaa/)

Fecha de publicación:
12
2005
Número de autores
7
Número de autores del IAC
0
Número de citas
1
Número de citas referidas
1
Descripción
Starforming galaxies with compact morphology and high optical luminosity (LBCGs) are very common at redshitfs z = 0.4 - 1.2. Those galaxies are believed to have evolved more than other galaxy class during the last ~ 8 Gyr, and are a mayor contributor to the global star formation rate density of the universe at z ~ 1. A robust way to gauge their evolution is throught quantities that do not change much when the star formation activity ceases. In this poster we present the stellar mass measurements for a sample of 30 LBCGs from the GOYA photometric survey. The stellar masses are obtained by fitting the photometry in UBVIJK filters to a two component galaxy population model obtained with GISSELXXI.
Tipo
Sin árbitro
Galaxias
Formación estelar

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