Add to ORKGWe present an initial survey of Mg II absorption characteristics in a carefully constructed, volume-limited subsample of the Sloan Digital Sky Survey. We survey quasars near nine z 0.11 luminous with the LRIS-B spectrograph on the Keck telescope. Only 2/9 exhibit strong MgII absorption at the galaxy's redshift [EW(2796) > 0.3 Å]. The two absorbers are among the bluest galaxies and are also relatively isolated. The results strongly suggest that MgII halo gas absorption in the local universe occurs preferentially around isolated blue galaxies with ongoing star formation
We constructed a sample of 205 galaxies (0.1 < z < 1.1) having extended CGM gas measured with MgII d...
We map the radial and azimuthal distribution of MgII gas within similar to 200 kpc (physical) of sim...
We present a study of strong intervening absorption systems in the near-IR spectra of 31 luminous qu...
We present an initial survey of Mg II absorption characteristics in the halos of a carefully constru...
The largest catalog of strong MgII absorbers to date derived from the Sloan Digital Sky Survey (SDSS...
This dissertation consists of several projects designed to further our understanding of galaxies and...
We study the properties of 1880 Mg II absorption line systems using only the photometric data catalo...
Using a sample of nearly 700 quasars with strong (W_0(2796)>0.8 Angstrom) MgII absorption lines dete...
The current status and remaining questions of Mgii absorbers are reviewed with an eye toward new res...
The current status and remaining questions of MgII absorbers are reviewed with an eye toward new res...
We describe the Mg II Absorber-Galaxy Catalog, MAGIICAT, a compilation of 182 spectroscopically iden...
We present the results from a spectroscopic survey for intervening MgII absorption in the spectra of...
We present the following results of photoionization modeling of six MgII-selected absorption systems...
International audienceWe present nebular emission associated with 198 strong Mg II absorbers at 0.35...
International audienceIn this paper we will present findings on the detection of Magnesium II (MgII,...
We constructed a sample of 205 galaxies (0.1 < z < 1.1) having extended CGM gas measured with MgII d...
We map the radial and azimuthal distribution of MgII gas within similar to 200 kpc (physical) of sim...
We present a study of strong intervening absorption systems in the near-IR spectra of 31 luminous qu...
We present an initial survey of Mg II absorption characteristics in the halos of a carefully constru...
The largest catalog of strong MgII absorbers to date derived from the Sloan Digital Sky Survey (SDSS...
This dissertation consists of several projects designed to further our understanding of galaxies and...
We study the properties of 1880 Mg II absorption line systems using only the photometric data catalo...
Using a sample of nearly 700 quasars with strong (W_0(2796)>0.8 Angstrom) MgII absorption lines dete...
The current status and remaining questions of Mgii absorbers are reviewed with an eye toward new res...
The current status and remaining questions of MgII absorbers are reviewed with an eye toward new res...
We describe the Mg II Absorber-Galaxy Catalog, MAGIICAT, a compilation of 182 spectroscopically iden...
We present the results from a spectroscopic survey for intervening MgII absorption in the spectra of...
We present the following results of photoionization modeling of six MgII-selected absorption systems...
International audienceWe present nebular emission associated with 198 strong Mg II absorbers at 0.35...
International audienceIn this paper we will present findings on the detection of Magnesium II (MgII,...
We constructed a sample of 205 galaxies (0.1 < z < 1.1) having extended CGM gas measured with MgII d...
We map the radial and azimuthal distribution of MgII gas within similar to 200 kpc (physical) of sim...
We present a study of strong intervening absorption systems in the near-IR spectra of 31 luminous qu...