Damped Lyα absorbers (DLAs) are a well-studied class of absorption line systems, and yet the properties of their host galaxies remain largely unknown. To investigate the origin of these systems, we have conducted an imaging survey of 32 quasar fields with intervening DLAs between z ∼ 1.9 and 3.8, leveraging a technique that allows us to image galaxies at any small angular separation from the background quasars. In this paper, we present the properties of the targeted DLA sample, new imaging observations of the quasar fields, and the analysis of new and archival spectra of the background quasars
Motivated by the discovery of rare enormous Lyman α nebulae (ELAN) around z ∼ 2 quasars, we initiate...
We present results on the clustering of Lyman break galaxies (LBGs) around a probable damped Lyα abs...
We present a study of the galaxy environment of 9 strong H I+C IV absorption line systems (16.2 < lo...
We report the detection of the host galaxy of a damped Lyα system (DLA) with log N(H I) [cm−2 ] = 2...
Using galaxies as background light sources to map the Lya absorption lines is a novel approach to st...
We review the current state of knowledge of damped Lyα systems (DLAs) selected in absorption on quas...
We present new observations acquired with the Multi Unit Spectroscopic Explorer instrument on the Ve...
We are exploring the connection between Damped Ly-α Absorption systems and Lyman Break Galaxies usin...
We have identified galaxies near two quasars that are at the redshift of damped Lyα (DLA) systems in...
We present deep imaging in the U, B and I bands obtained under excellent seeing conditions of the do...
We present results from a survey designed to probe the star formation properties of 32 damped Lyman ...
peer reviewedLe Brun et al. (1997) presented the first identifications of the galaxies giving rise t...
We present results from a survey of galaxies in the elds of six z 3 Damped Lyman systems (DLAs) u...
We demonstrate that the UV brightest quasars at z = 1–2 live in overdense environments. This is base...
We study the distribution and dynamics of the circumgalactic and intergalactic medium using a dense ...
Motivated by the discovery of rare enormous Lyman α nebulae (ELAN) around z ∼ 2 quasars, we initiate...
We present results on the clustering of Lyman break galaxies (LBGs) around a probable damped Lyα abs...
We present a study of the galaxy environment of 9 strong H I+C IV absorption line systems (16.2 < lo...
We report the detection of the host galaxy of a damped Lyα system (DLA) with log N(H I) [cm−2 ] = 2...
Using galaxies as background light sources to map the Lya absorption lines is a novel approach to st...
We review the current state of knowledge of damped Lyα systems (DLAs) selected in absorption on quas...
We present new observations acquired with the Multi Unit Spectroscopic Explorer instrument on the Ve...
We are exploring the connection between Damped Ly-α Absorption systems and Lyman Break Galaxies usin...
We have identified galaxies near two quasars that are at the redshift of damped Lyα (DLA) systems in...
We present deep imaging in the U, B and I bands obtained under excellent seeing conditions of the do...
We present results from a survey designed to probe the star formation properties of 32 damped Lyman ...
peer reviewedLe Brun et al. (1997) presented the first identifications of the galaxies giving rise t...
We present results from a survey of galaxies in the elds of six z 3 Damped Lyman systems (DLAs) u...
We demonstrate that the UV brightest quasars at z = 1–2 live in overdense environments. This is base...
We study the distribution and dynamics of the circumgalactic and intergalactic medium using a dense ...
Motivated by the discovery of rare enormous Lyman α nebulae (ELAN) around z ∼ 2 quasars, we initiate...
We present results on the clustering of Lyman break galaxies (LBGs) around a probable damped Lyα abs...
We present a study of the galaxy environment of 9 strong H I+C IV absorption line systems (16.2 < lo...