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

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

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005rmxac..24..227c&link_type=abstract

II International GTC Workshop: Science with GTC 1st-light Instruments and the LMT (Eds. A. M. Hidalgo-Gámez, J. J. González, J.

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Galaxies: Evolution, Galaxies: Star Formation

Scientific paper

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.

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