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We report observations of four sub-damped Lyman-alpha (sub-DLA) quasar absorbers at z<0.5 obtained with the Hubble Space Telescope Cosmic Origins Spectrograph. We measure the available neutrals or ions of C, N, O, Si, P, S, Ar, Mn, Fe,…

宇宙学与河外天体物理 · 物理学 2015-06-11 Debopam Som , Varsha P. Kulkarni , Joseph Meiring , Donald G. York , Celine Péroux , James T. Lauroesch , Monique C. Aller , Pushpa Khare

We present a new study of the effects of quasar obscuration on the statistics of Damped Ly alpha (DLA) systems. We show that the extinction of any Galactic or extragalactic HI region increases with the column density of zinc with a turning…

天体物理学 · 物理学 2009-11-10 Giovanni Vladilo , Celine Peroux

We present the chemical abundance measurements of the first large, medium-resolution, uniformly selected damped Lyman alpha system (DLA) survey. The sample contains 99 DLAs towards 89 quasars selected from the SDSS DR5 DLA sample in a…

宇宙学与河外天体物理 · 物理学 2015-06-16 Regina A. Jorgenson , Michael T. Murphy , Rodger Thompson

The effects of the dust on the determination of elemental abundances in damped Ly alpha (DLA) absorbers are investigated. Relations between the observed abundances measured in the gas phase and the overall abundances (gas plus dust) are…

天体物理学 · 物理学 2009-10-30 Giovanni Vladilo

We present high-resolution UES spectra of the quasar PHL 957 obtained for studying the foreground Damped Ly-alpha galaxy at z=2.309. Measurements of absorption lines lead to accurate abundance determinations of Fe, S and N which complement…

天体物理学 · 物理学 2009-10-30 Paolo Molaro , Miriam Centurion , Giovanni Vladilo

We use the existing catalog of Damped Lyman-Alpha (DLA) systems to place constraints on the amount of evolution in the baryonic content of galaxies and on the value of the cosmological constant. The density of cold gas at redshifts z=3+-1…

天体物理学 · 物理学 2007-05-23 Eric Woods , Abraham Loeb

We report Keck/ESI and VLT/UVES observations of three super-damped Lyman-alpha quasar absorbers with H I column densities log N(HI) >= 21.7 at redshifts z=2-2.5. All three absorbers show similar metallicities (-1.3 to -1.5 dex), and dust…

星系天体物理 · 物理学 2015-12-09 Varsha P. Kulkarni , Debopam Som , Sean Morrison , Celine Peroux , Samuel Quiret , Donald G. York

We report the discovery and analysis of the most metal-poor damped Lyman-alpha (DLA) system currently known, based on observations made with the Keck HIRES spectrograph. The metal paucity of this system has only permitted the determination…

宇宙学与河外天体物理 · 物理学 2017-01-13 Ryan Cooke , Max Pettini , Charles C. Steidel

We report on the results of a search for CO(3-2) emission from the galaxy counterpart of a high-metallicity Damped Ly-alpha Absorber (DLA) at z=2.5832 towards the quasar Q0918+1636. We do not detect CO emission from the previously…

We present a measurement of the D/H abundance ratio in a metal-poor damped Lyman alpha (DLA) system along the sightline of QSO SDSS1558-0031. The DLA system is at redshift z = 2.70262, has a neutral column density of log(NHI)=20.67+/-0.05…

Detailed studies of Damped and sub-Damped Lyman-alpha systems (DLA), the galaxies probed by the absorption they produce in the spectra of background quasars, rely on identifying the galaxy responsible for the absorber with more traditional…

宇宙学与河外天体物理 · 物理学 2015-05-19 Celine Peroux , Nicolas Bouche , Varsha P. Kulkarni , Donald G. York , Giovanni Vladilo

We present a spectroscopic study of six damped Lya absorption (DLA) systems at z<0.65, based on moderate-to-high resolution spectra of the galaxies responsible for the absorbers. Combining known metallicity measurements of the absorbers…

天体物理学 · 物理学 2009-11-10 Hsiao-Wen Chen , Robert C. Kennicutt , Michael Rauch

We present a detailed analysis of chemical abundances in a sub-damped Lyman alpha absorber at z=1.839 towards the quasar B1101-26, based on a very-high-resolution (R ~ 75,000) and high-signal-to-noise (S/N >100) spectrum observed with the…

星系天体物理 · 物理学 2014-12-10 Anne Fox , Philipp Richter , Cora Fechner

We report here a study of nitrogen and $\alpha$-capture element (O, S, and Si) abundances in 18 Damped Ly$\alpha$ Absorbers (DLAs) and sub-DLAs drawn from the ESO-UVES Advanced Data Products (EUADP) database. We report 9 new measurements, 5…

We have investigated chemical evolution in the young universe by analysing the detailed chemical enrichment pattern of a metal-rich galaxy at high redshift. The recent detection of over 20 elements in the gas-phase of a damped Lyman-alpha…

天体物理学 · 物理学 2009-11-10 Yeshe Fenner , Jason X. Prochaska , Brad K. Gibson

We present a detailed high spectral resolution (R $\sim$ 40000) study of five high-z damped Lyman $\alpha$ systems (DLAs) and one sub-DLA detected along four QSO sightlines. Four of these DLAs are very metal-poor with [Fe/H] $\le$ $-$2. One…

星系天体物理 · 物理学 2015-06-18 R. Dutta , R. Srianand , H. Rahmani , P. Petitjean , P. Noterdaeme , C. Ledoux

We report the discovery of the first 'ghostly' damped Ly$\alpha$ absorption system (DLA), which is identified by the presence of absorption from strong low-ion species at $z_{\rm abs}=1.70465$ along the line of sight to the quasar…

Damped Ly-alpha absorbers (DLAs) can be used to measure gas-phase metallicities at large cosmological lookback times with high precision. Relative abundances can still be measured accurately deep into the reionization epoch (z > 6) using…

宇宙学与河外天体物理 · 物理学 2015-06-12 Girish Kulkarni , Emmanuel Rollinde , Joseph F. Hennawi , Elisabeth Vangioni

We use cosmological smoothed-particle hydrodynamics (SPH) simulations of the Lambda cold dark matter (CDM) model to study the abundance of damped Lyman-alpha absorbers (DLAs) in the redshift range z=0-4.5. We compute the cumulative DLA…

天体物理学 · 物理学 2008-11-26 Kentaro Nagamine , Volker Springel , Lars Hernquist

We present the direct detection of molecular hydrogen at the highest redshift known today (z_abs=4.224) in a Damped Lyman-alpha (DLA) system toward the quasar PSS J1443+2724. This absorber is remarkable for having one of the highest…

天体物理学 · 物理学 2009-11-11 C. Ledoux , P. Petitjean , R. Srianand