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Properties of Hα-selected star-forming galaxies from z ∼ 0.8 to now

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2005

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Instituto de Astronomía de la UNAM
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We present a long-term project to study the characteristics and evolution of current star-forming galaxies at different redshifts. Our results support the idea that the higher Star Formation Density measured at redshift z=0.24 is due to an increase of the density of bursting galaxies and not to an intrinsic change on overall galaxy properties.

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© 2005 Instituto de Astronomía, UNAM. International GTC Workshop - Science with GTC 1st-Light Instruments and the LMT (2nd. 2005. Mexico City/Mexico).

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