activity
20012009
most citedA Population of Faint Extended Line Emitters and the Host Galaxies of Optically Thick QSO Absorption Systems

234 citations · 1.2k across the 17 of their papers we have counts for

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Showing 2003 · astro-phShow all

6 papers · 2 filters

astro-ph2003

CIV Absorbers in z>4 Quasars: Tracing Early Galactic Halos Evolution

Celine Peroux, Patrick Petitjean, Bastien Aracil +2

We use 29 z>4 quasar spectra to build a homogeneous sample of high-redshift CIV absorbers. We use these data to calculate the number density, n(z), of W_rest(CIV)>0.30 A CIV double…

astro-ph200317 cited

Investigating lensing by absorbers in the 2dF-Quasar survey

Brice Ménard, Céline Péroux

We use the first data release of the 2-degree Field Quasar survey to investigate the effect of gravitational magnification by foreground absorbing systems on background quasars. We…

astro-ph2003

Nitrogen Abundances in High-z DLAs

P. Molaro, M. Centurion, V. D'Odorico +1

Determination of chemical abundances for elements produced mainly by Type I SNae and intermediate mass stars in high redshift DLAs probes the early chemical build-up on time-scales…

astro-ph2003

A Homogeneous Sample of Sub-DLAs II: Statistical, Kinematic and Chemical Properties

Celine Peroux, Miroslava Dessauges-Zavadsky, Sandro D'Odorico +2

Damped Ly-alpha Systems (DLAs), with N(HI)>2*10^20 cm^{-2}, observed in quasars have allowed us to quantify the chemical content of the Universe over cosmological scales. Such stud…

astro-ph2003

A Homogeneous Sample of Sub-DLAs I: Construction of the Sample and Chemical Abundance Measurements

M. Dessauges-Zavadsky, C. Peroux, T. -S. Kim +2

In this first paper of a series, we report on the use of quasar spectra obtained with the UVES high resolution spectrograph and available through the ESO VLT archive to build the f…

astro-ph2003

Ar I as a tracer of ionization evolution

Giovanni Vladilo, Miriam Centurion, Valentina D'Odorico +1

We present a study of Ar abundances in 15 damped Ly alpha systems (DLAs) in the redshift interval from 2.3 to 3.4. The sample includes 4 new UVES/VLT measurements of Ar I column de…