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Related papers: Neutral gas density in Damped Lyman Alpha systems

200 papers

We report {\it HST} COS spectroscopy of 10 quasars with foreground star-forming galaxies at 0.02$<$$z$$<$ 0.14 within impact parameters of $\sim$1-7 kpc. We detect damped/sub-damped Ly$\alpha$ absorption in 100$\%$ of cases where no…

We analyzed the spectroscopic and photometric database of the 5th data release of the Sloan Digital Sky Survey (SDSS) to search for evidence of the quasar reddening produced by dust embedded in intervening damped Ly alpha (DLA) systems.…

Astrophysics · Physics 2009-11-13 Giovanni Vladilo , Jason X. Prochaska , Arthur M. Wolfe

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…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-16 Regina A. Jorgenson , Michael T. Murphy , Rodger Thompson

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…

Cosmology and Nongalactic Astrophysics · Physics 2017-01-13 Ryan Cooke , Max Pettini , Charles C. Steidel

We present the results from a damped Lya survey of the Sloan Digital Sky Survey, Data Release 3 based on over 500 new damped Lya systems at z>2.2. We measure the HI column density distribution f(N) and its zeroth and first moments (the…

Astrophysics · Physics 2008-11-26 Jason X. Prochaska , Stephane Herbert-Fort , Arthur M. Wolfe

We present HIRES observations for 30 damped Lyman alpha systems, selected on the basis of their large metal column densities from previous, lower resolution data. The measured metal column densities for Fe, Zn, S, Si, Cr, Mn, and Ni are…

Astrophysics of Galaxies · Physics 2015-06-23 Trystyn A. M. Berg , Marcel Neeleman , J. Xavier Prochaska , Sara L. Ellison , Arthur M. Wolfe

We have obtained high signal:to:noise optical spectroscopy at 5\AA\ resolution of 27 quasars from the APM z$>$4 quasar survey. The spectra have been analyzed to create new samples of high redshift Lyman-limit and damped Lyman-$\alpha$…

Astrophysics · Physics 2007-05-23 L. J. Storrie-Lombardi , R. G. McMahon , M. J. Irwin , C. Hazard

We report new HST and ground-based observations of a damped Lyman-alpha absorption system toward the QSO 0850+4400. The redshift of the absorption system is z = 0.163770 and the neutral hydrogen column density of the absorption system is…

By combining our UVES-VLT spectra of a sample of four damped Ly-alpha systems (DLAs) toward the quasars Q0100+13, Q1331+17, Q2231-00 and Q2343+12 with the existing HIRES-Keck spectra, we covered the total spectral range from 3150 to 10000 A…

Astrophysics · Physics 2009-11-10 M. Dessauges-Zavadsky , F. Calura , J. X. Prochaska , S. D'Odorico , F. Matteucci

We calculate in detail the expected properties of low redshift DLA systems under the assumption that they arise in the gaseous disks of galaxies like those in the z=0 population. A sample of 355 nearby galaxies is analysed, for which high…

We study the average Ly$\alpha$ emission associated with high-$z$ strong (log $N$(H I) $\ge$ 21) damped Ly$\alpha$ systems (DLAs). We report Ly$\alpha$ luminosities ($L_{\rm Ly\alpha}$) for the full as well as various sub-samples based on…

Astrophysics of Galaxies · Physics 2016-12-14 Ravi Joshi , Raghunathan Srianand , Pasquier Noterdaeme , Patrick Petitjean

In this work, we study argon abundances in the interstellar medium of high-redshift galaxies (2<z(abs)<4.2) detected as Damped Lya absorbers (DLA) in the spectra of background quasars. We use high-resolution quasar spectra obtained from the…

Using a sample of 100 H I - selected damped Lyman alpha (DLA) systems, observed with the High Resolution Echelle Spectrometer on the Keck I telescope, we present evidence that the scatter in the well-studied correlation between the redshift…

Cosmology and Nongalactic Astrophysics · Physics 2013-05-07 Marcel Neeleman , Arthur M. Wolfe , J. Xavier Prochaska , Marc Rafelski

Any viable cosmological model must produce enough structure at early epochs to explain the amount of gas associated with high-redshift damped Ly$\alpha$ systems. We study the evolution of damped Ly$\alpha$ systems at redshifts $z\ge 2$ in…

Astrophysics · Physics 2009-10-30 Chung-Pei Ma , Edmund Bertschinger , Lars Hernquist , David H. Weinberg , Neal Katz

Images of five QSO fields containing six damped Lyman alpha (DLA) systems at redshifts 0.09<z<0.53 are presented. Identifications for the DLA galaxies giving rise to the DLA systems are made. The observed and modeled characteristics of the…

We review the analytical prescriptions in the literature to model the 21-cm (emission line surveys/intensity mapping experiments) and Damped Lyman-Alpha (DLA) observations of neutral hydrogen (HI) in the post-reionization universe. While…

Cosmology and Nongalactic Astrophysics · Physics 2017-08-23 Hamsa Padmanabhan , T. Roy Choudhury , Alexandre Refregier

We have combined new high resolution UVES-VLT observations of a sample of four damped Ly-alpha systems (DLAs) at redshifts between z_abs = 1.7-2.5 with the existing HIRES-Keck spectra to undertake a comprehensive study of their physical…

Astrophysics · Physics 2009-11-07 M. Dessauges-Zavadsky , J. X. Prochaska , S. D'Odorico

Damped Lyman alpha systems seen in the spectra of high-z QSOs arise in high-density neutral gas in which molecular hydrogen (H_2) should be conspicuous. Systematic searches to detect the H_2 lines redshifted into the Lyman alpha forest at…

Astrophysics · Physics 2007-05-23 R. Srianand , P. Petitjean , C. Ledoux

(ABRIDGED) We present a study of the highly ionized gas (plasma) associated with damped Lyman-alpha (DLA) systems at z=2.1-3.1. We search for O VI absorption and corresponding Si IV, C IV, and N V in a Very Large…

Astrophysics · Physics 2009-11-13 Andrew J. Fox , Patrick Petitjean , Cedric Ledoux , Raghunathan Srianand

We have identified a metal-strong (logN(Zn+) > 13.15 or logN(Si+) > 15.95) DLA (MSDLA) population from an automated quasar (QSO) absorber search in the Sloan Digital Sky Survey Data Release 3 (SDSS-DR3) quasar sample, and find that MSDLAs…