activity
20022012
most citedThe dominant role of mergers in the size evolution of massive early-type galaxies since z ~ 1

152 citations · 386 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2012★ 33 cited

Comparison of star formation rates from Halpha and infrared luminosities as seen by Herschel

H. Domínguez, M. Mignoli, F. Pozzi +55

We empirically test the relation between the SFR(LIR) derived from the infrared luminosity, LIR, and the SFR(Ha) derived from the Ha emission line luminosity using simple conversio…

astro-ph.CO2012★ 152 cited

The dominant role of mergers in the size evolution of massive early-type galaxies since z ~ 1

C. López-Sanjuan, O. Le Fèvre, O. Ilbert +60

In this paper we measure the merger fraction and rate, both minor and major, of massive early-type galaxies (M_star >= 10^11 M_Sun) in the COSMOS field, and study their role in mas…

astro-ph.CO2011★ 67 cited

The evolution of quiescent galaxies at high redshift (z > 1.4)

H. Domínguez Sánchez, F. Pozzi, C. Gruppioni +45

We have studied the evolution of high redshift quiescent galaxies over an effective area of ~1.7 deg^2 in the COSMOS field. Galaxies have been divided according to their star-forma…

astro-ph2005★ 134 cited

A comparative analysis of empirical calibrators for nebular metallicity

Enrique Perez-Montero, Angeles I. Diaz

We present a new analysis of the main empirical calibrators of oxygen abundance for ionised gas nebulae. With that aim we have compiled an extensive sample of objects with emission…

astro-ph2004

Ionising stellar populations in circumnuclear star forming regions

Enrique Perez-Montero, Angeles I. Diaz, Marcelo Castellanos

We present a study of the stellar populations and gas physical conditions in Circumnuclear Star Forming Regions (CNSFRs) based on spectrophotometric data, including the 7000 angstr…

astro-ph2002

Optical and near IR spectroscopy of low excitation HII regions with GTC

Enrique Perez-Montero, Marcelo Castellanos, Angeles I. Diaz

The determination of chemical abundances in ionized gas nebulae is based on the detection of auroral emission lines, from which it is possible to deduce the line temperatures of se…