Showing 1–20 of 143 results
/ Date/ Name
May 17, 2012Search for cold gas in strong MgII absorbers at 0.5<z<1.5: nature and evolution of 21-cm absorbersMay 10, 2012Metallicities, dust and molecular content of a QSO-Damped Lyman-α system reaching log N (H i) = 22: An analog to GRB-DLAsAug 11, 2009Evolution of the cosmological mass density of neutral gas from Sloan Digital Sky Survey II - Data Release 7Sep 4, 2008Detection of the 2175Å~ extinction feature and 21-cm absorption in two MgII systems at z~1.3Sep 22, 2008HD molecules at high redshift: A low astration factor of deuterium in a solar-metallicity DLA system at z=2.418Jul 22, 2013The UVES Large Program for Testing Fundamental Physics II: Constraints on a Change in μ Towards Quasar HE 0027-1836Feb 12, 2014A study of low-metallicity DLAs at high redshift and C II* as a probe of their physical conditionsDec 31, 2020Physical conditions and redshift evolution of optically thin C III absorbers: Low-z sampleMar 17, 2021Evolution of cold gas at 2<z<5: a blind search for HI and OH absorption lines towards mid-infrared color selected radio-loud AGNsApr 3, 1998Molecules in the $z_{\rm abs}$~=~2.8112 damped system toward PKS~0528--250Nov 23, 2000Molecular hydrogen and the nature of damped Lyman-alpha systemsMar 21, 2000Physical conditions in broad and associated narrow absorption-line systems toward APM 08279+5255Nov 2, 2007On the enhanced cosmic-ray ionization rate in the diffuse cloud towards Zeta PerseiApr 1, 2008First detection of CO in a high-redshift DLAApr 27, 2015Neutral atomic-carbon QSO absorption-line systems at z>1.5: Sample selection, HI content, reddening, and 2175 A extinction featureAug 19, 201321-cm absorption from galaxies at z ~ 0.3Jun 20, 2022Mapping HI 21-cm in the Klemola 31 group at z = 0.029: emission and absorption towards PKS2020-370Jul 24, 2011Partial coverage of the Broad Line Region of Q1232+082 by an intervening H2-bearing cloudAug 31, 2009SDSS J092712.64+294344.0: recoiling black hole or merging galaxies?Sep 5, 2014The UVES Large Program for testing fundamental physics - III. Constraints on the fine-structure constant from 3 telescopes