We have studied in detail the properties of local active star-forming galaxies from the UCM survey, and in particular their star-formation histories. We have quantified the relative importance of the current episode of star formation in comparison to the underlying older stellar populations. We have also determined the total stellar mass function and burst mass function for the UCM sample using the M/L calculated for each galaxy. Integrating this mass function we obtained the contribution of the star-forming galaxies to the total stellar mass density of the local Universe
International audienceThis paper presents the spatially resolved star formation history (SFH) of nea...
International audienceWe present measurements of the stellar mass functions (SMFs) of star-forming a...
The measurement of the star formation rate density of the universe is of prime importance in underst...
We present the integrated properties of the stellar populations in the Universidad Complutense de Ma...
We present the optical and near-infrared luminosity and mass functions of the local star-forming gal...
The Universidad Complutense de Madrid (UCM) survey is a long-term project aimed at finding and analy...
We present a photometric study of the Halpha emission in the Universidad Complutense de Madrid (UCM)...
We present an analysis of the integrated properties of the stellar populations in the Universidad Co...
We present new near-infrared J and K imaging data for 67 galaxies from the Universidad Complutense d...
A spectroscopic analysis of the entire sample of Ha emission-line galaxies (ELGs) contained in lists...
The Universidad Complutense de Madrid survey is a long-term project with the aim of finding and anal...
The spatially resolved stellar population content of today’s galaxies holds important information fo...
Observations have revealed a bimodality in galaxy properties such as color and morphology leading to...
We present the CIDA-UCM-Yale (Centro de Investigaciones de Astronomia, Universidad Complutense de Ma...
© ESO, 2016. The spatially resolved stellar population content of today's galaxies holds important i...
International audienceThis paper presents the spatially resolved star formation history (SFH) of nea...
International audienceWe present measurements of the stellar mass functions (SMFs) of star-forming a...
The measurement of the star formation rate density of the universe is of prime importance in underst...
We present the integrated properties of the stellar populations in the Universidad Complutense de Ma...
We present the optical and near-infrared luminosity and mass functions of the local star-forming gal...
The Universidad Complutense de Madrid (UCM) survey is a long-term project aimed at finding and analy...
We present a photometric study of the Halpha emission in the Universidad Complutense de Madrid (UCM)...
We present an analysis of the integrated properties of the stellar populations in the Universidad Co...
We present new near-infrared J and K imaging data for 67 galaxies from the Universidad Complutense d...
A spectroscopic analysis of the entire sample of Ha emission-line galaxies (ELGs) contained in lists...
The Universidad Complutense de Madrid survey is a long-term project with the aim of finding and anal...
The spatially resolved stellar population content of today’s galaxies holds important information fo...
Observations have revealed a bimodality in galaxy properties such as color and morphology leading to...
We present the CIDA-UCM-Yale (Centro de Investigaciones de Astronomia, Universidad Complutense de Ma...
© ESO, 2016. The spatially resolved stellar population content of today's galaxies holds important i...
International audienceThis paper presents the spatially resolved star formation history (SFH) of nea...
International audienceWe present measurements of the stellar mass functions (SMFs) of star-forming a...
The measurement of the star formation rate density of the universe is of prime importance in underst...