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20032008
most citedLensing, reddening and extinction effects of MgII absorbers from z=0.4 to z=2

101 citations · 300 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph200817 cited

Deep optical spectroscopy of extended Lyman alpha emission around three radio-quiet z=4.5 quasars

F. Courbin, P. North, A. Eigenbrod +1

We report the first results of a spectroscopic search for Lyman alpha, envelopes around three z=4.5 radio-quiet quasars. Our observational strategy uses the FORS2 spectrograph atta…

astro-ph200883 cited

On the HI content, dust-to-gas ratio and nature of MgII absorbers

Brice Ménard, Doron Chelouche

We estimate the mean dust-to-gas ratio of MgII absorbers as a function of rest equivalent width W_0 and redshift over the range 0.5<z<1.4. Using the expanded SDSS/HST sample of low…

astro-ph200769 cited

The Dust Content of Galaxy Clusters

Doron Chelouche, Benjamin P. Koester, David V. Bowen

We report on the detection of reddening toward z ~ 0.2 galaxy clusters. This is measured by correlating the Sloan Digital Sky Survey cluster and quasar catalogs and by comparing th…

astro-ph200730 cited

On the Connection Between Metal Absorbers and Quasar Nebulae

Doron Chelouche, Brice Ménard, David V. Bowen +1

We establish a simple model for the distribution of cold gas around L* galaxies using a large set of observational constraints on the properties of strong MgII absorber systems. Ou…

astro-ph2007101 cited

Lensing, reddening and extinction effects of MgII absorbers from z=0.4 to z=2

Brice Ménard, Daniel Nestor, David Turnshek +5

Using a sample of almost 7000 strong MgII absorbers with 0.4 < z < 2.2 detected in the SDSS DR4 dataset, we investigate the gravitational lensing and dust extinction effects they i…

astro-ph2003

The Properties and the Evolution of the Highly Ionized Gas in MR2251-178

S. Kaspi, H. Netzer, D. Chelouche +3

We present the first XMM-Newton observations of the radio-quiet quasar MR2251-178. We model the X-ray spectrum with two power laws, one at high energies with a slope of Γ=1.6 and t…