The rare close projection of two quasars on the sky provides the opportunity to study the host galaxy environment of a foreground quasar in absorption against the continuum emission of a background quasar. For over a decade the "Quasars probing quasars" series has utilized this technique to further the understanding of galaxy formation and evolution in the presence of a quasar at z > 2, resolving scales as small as a galactic disk and from bound gas in the circumgalactic medium to the diffuse environs of intergalactic space. Presented here is the public release of the quasar pair spectral database utilized in these studies. In addition to projected pairs at z > 2, the database also includes quasar pair members at z < 2, gravitational lens c...
We conducted an exploratory search for quasars at z ~ 6-8, using the Early Data Release (EDR) from t...
peer reviewedHigh-redshift binary quasars provide key insights into mergers and quasar activity, and...
We present the first results from our survey of intervening and proximate Lyman limit systems (LLSs)...
The rare close projection of two quasars on the sky provides the opportunity to study the host galax...
Quasars are the most luminous type of active galactic nuclei and their study is fundamental to shed ...
We present the first results from our survey of intervening and proximate Lyman limit systems (LLSs)...
Models of galaxy formation make the most direct predictions on gas related processes. Specifically, ...
We obtained medium-resolution spectra of 336 quasar candidates in the COSMOS HST Treasury field usin...
Context. Quasi-stellar objects (quasars) located behind nearby galaxies provide an excellent absolut...
Although quasar spectra appear remarkably similar, subtle systematic differences are well- known and...
We demonstrate that the UV brightest quasars at z = 1–2 live in overdense environments. This is base...
I present the data for an optical/near-infrared study of radio-loud quasar environments from z = 0.6...
We present the results of long-slit CCD spectroscopy on 39 objects and four close companions from th...
The Sloan Digital Sky Survey has obtained images in five broad-band colors for several hundred squar...
We report the serendipitous discoveries of companion galaxies to two high-redshift quasars. SDSS J02...
We conducted an exploratory search for quasars at z ~ 6-8, using the Early Data Release (EDR) from t...
peer reviewedHigh-redshift binary quasars provide key insights into mergers and quasar activity, and...
We present the first results from our survey of intervening and proximate Lyman limit systems (LLSs)...
The rare close projection of two quasars on the sky provides the opportunity to study the host galax...
Quasars are the most luminous type of active galactic nuclei and their study is fundamental to shed ...
We present the first results from our survey of intervening and proximate Lyman limit systems (LLSs)...
Models of galaxy formation make the most direct predictions on gas related processes. Specifically, ...
We obtained medium-resolution spectra of 336 quasar candidates in the COSMOS HST Treasury field usin...
Context. Quasi-stellar objects (quasars) located behind nearby galaxies provide an excellent absolut...
Although quasar spectra appear remarkably similar, subtle systematic differences are well- known and...
We demonstrate that the UV brightest quasars at z = 1–2 live in overdense environments. This is base...
I present the data for an optical/near-infrared study of radio-loud quasar environments from z = 0.6...
We present the results of long-slit CCD spectroscopy on 39 objects and four close companions from th...
The Sloan Digital Sky Survey has obtained images in five broad-band colors for several hundred squar...
We report the serendipitous discoveries of companion galaxies to two high-redshift quasars. SDSS J02...
We conducted an exploratory search for quasars at z ~ 6-8, using the Early Data Release (EDR) from t...
peer reviewedHigh-redshift binary quasars provide key insights into mergers and quasar activity, and...
We present the first results from our survey of intervening and proximate Lyman limit systems (LLSs)...