Artículo de publicación ISIWe present FWHM = 5 to 8 Angstrom optical spectra of nine previously unknown quasars (QSOs) drawn from the Calan/Tololo Survey. We have chosen this sample based on QSO redshift, z > 3, and the presence of either candidate damped Ly alpha (DLA) or Lyman-limit (LL) systems in their. spectra. The spectra show at least 9 DLA systems at redshifts: 2.25 < z < 3.26, which are identified by the shape and strength of the HI-Ly alpha absorption line, by the presence of Ly beta and low-ionization metal lines at the same redshift, and in most cases: by the observed Lyman-break. We thus provide the astronomical community with new interesting: targets for high resolution spectroscopy oil large telescopes. We describe all the sp...
We report the first results of a spectroscopic search for Ly alpha envelopes around three z similar ...
We report preliminary results from a targeted investigation on quasars containing damped Lyman-alpha...
Quasar absorption lines have long been recognised to be a sensitive probe of the abundances, physica...
Artículo de publicación ISIWe present FWHM = 5 to 8 Angstrom optical spectra of nine previously unkn...
We present $FWHM = 5$ to 8 Å optical spectra of nine previously unknown quasars (QSOs) drawn from th...
We have completed spectroscopic observations using LRIS on the Keck 1 telescope of 30 very high reds...
The APM multicolor survey for bright z > 4 objects, covering 2500 deg^2 of sky to m_r ~ 19, resulted...
We present results from observations of the QSO field J2342+34 as part of a systematic survey for Ly...
New intermediate-resolution spectroscopy for six members of a sample of 68 moderate- to high-redshif...
The APM multicolor survey for bright z > 4 objects, covering 2500 deg^2 of sky to m(R)~19, resulted ...
We present high signal-to-noise, ~5 Å resolution (FWHM) spectra of 66 z ≳ 4 bright quasars obtained ...
The discovery of a z_abs = 0.0912 damped Lyman-alpha absorption-line system in the HST-FOS ultraviol...
We present Keck/LRIS spectra of a candidate damped Lyman-alpha (DLA) galaxy toward the QSO 3C196 (z_...
We present spectroscopic observations of six high redshift (z(em) > 2) quasars, which have been sele...
The number of damped Ly-alpha absorbers (DLAs) currently known is about 100, but our knowledge of th...
We report the first results of a spectroscopic search for Ly alpha envelopes around three z similar ...
We report preliminary results from a targeted investigation on quasars containing damped Lyman-alpha...
Quasar absorption lines have long been recognised to be a sensitive probe of the abundances, physica...
Artículo de publicación ISIWe present FWHM = 5 to 8 Angstrom optical spectra of nine previously unkn...
We present $FWHM = 5$ to 8 Å optical spectra of nine previously unknown quasars (QSOs) drawn from th...
We have completed spectroscopic observations using LRIS on the Keck 1 telescope of 30 very high reds...
The APM multicolor survey for bright z > 4 objects, covering 2500 deg^2 of sky to m_r ~ 19, resulted...
We present results from observations of the QSO field J2342+34 as part of a systematic survey for Ly...
New intermediate-resolution spectroscopy for six members of a sample of 68 moderate- to high-redshif...
The APM multicolor survey for bright z > 4 objects, covering 2500 deg^2 of sky to m(R)~19, resulted ...
We present high signal-to-noise, ~5 Å resolution (FWHM) spectra of 66 z ≳ 4 bright quasars obtained ...
The discovery of a z_abs = 0.0912 damped Lyman-alpha absorption-line system in the HST-FOS ultraviol...
We present Keck/LRIS spectra of a candidate damped Lyman-alpha (DLA) galaxy toward the QSO 3C196 (z_...
We present spectroscopic observations of six high redshift (z(em) > 2) quasars, which have been sele...
The number of damped Ly-alpha absorbers (DLAs) currently known is about 100, but our knowledge of th...
We report the first results of a spectroscopic search for Ly alpha envelopes around three z similar ...
We report preliminary results from a targeted investigation on quasars containing damped Lyman-alpha...
Quasar absorption lines have long been recognised to be a sensitive probe of the abundances, physica...