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Related papers: A Damped Ly-alpha Absorption-line System in an App…

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We present deep ground based imaging of the environments of five QSOs that contain sub-Damped Lyman-alpha systems at z<1 with the SOAR telescope and SOI camera. We detect a clear surplus of galaxies in these small fields, supporting the…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 Joseph D. Meiring , James T. Lauroesch , Lutz Haberzettl , Varsha P. Kulkarni , Celine Peroux , Pushpa Khare , Donald G. York

The Damped Lyman-alpha systems (DLAs), seen in absorption in the spectrum of quasars, are believed to contain a large fraction of the neutral gas in the Universe. Paradoxically, these systems are more difficult to observe at z_abs<1.7,…

Astrophysics · Physics 2009-11-10 Celine Peroux , Jean-Michel Deharveng , Vincent Le Brun , Stefano Cristiani

We present the detection of [OIII] emission lines from the galaxies responsible for two high-redshift z>1.75 damped Lyman-alpha (DLA) absorption lines. These are the first detections of rest-frame optical emission lines from high-redshift…

Astrophysics · Physics 2011-03-10 S. J. Weatherley , S. J. Warren , P. Moller , S. M. Fall , J. U. Fynbo , S. M. Croom

We have searched the Sloan Digital Sky Survey Data Release 12 for ghostly Damped Ly$\alpha$ (DLA) systems. These systems, located at the redshift of the quasars, show strong absorption from low-ionization atomic species but reveal no HI…

Astrophysics of Galaxies · Physics 2020-01-15 Hassan Fathivavsari

Ground based optical observations have yielded considerable information on the statistics of damped-lyman alpha systems. In particular these systems are known to be the dominant repository of the observed neutral gas at high redshift.…

Astrophysics · Physics 2016-01-27 Jayaram N. Chengalur , A. G. de Bruyn , R. Braun , C. L. Carilli

Reservoirs of dense atomic gas (primarily hydrogen), contain approximately 90 percent of the neutral gas at a redshift of 3, and contribute to 2-3 percent of the total baryons in the Universe. These damped Lyman-${\alpha}$ systems (so…

Damped Ly-alpha absorbers (DLAs) are a well-studied class of absorption line systems, and yet the properties of their host galaxies remain largely unknown. To investigate the origin of these systems, we have conducted an imaging survey of…

Astrophysics of Galaxies · Physics 2015-06-19 Michele Fumagalli , John M. O'Meara , J. Xavier Prochaska , Nissim Kanekar , Arthur M. Wolfe

We have identified galaxies near two quasars which are at the redshift of damped Lyman-alpha (DLA) systems in the UV spectra of the quasars. Both galaxies are actively forming stars. One galaxy has a luminosity close to the break in the…

In this paper we present Monte-Carlo simulations of Lyman alpha absorption systems which originate in galactic haloes, galaxy discs and dark matter (DM) satellites around big central haloes. It is found that for strong Lyman alpha…

Astrophysics · Physics 2009-10-31 W. P. Lin , G. Boerner , H. J. Mo

We report new observations of ZnII and CrII absorption lines in 10 damped \lya systems (DLAs), mostly at redshift $z_{abs} \simgt 2.5$ . By combining these results with those from our earlier survey (Pettini et al. 1994) and other recent…

Astrophysics · Physics 2015-06-24 Max Pettini , Linda J. Smith , David L. King , Richard W. Hunstead

The damped and sub-damped Lyman alpha systems (DLAs and sub-DLAs) traced in absorption against bright background quasars represent the main reserve of neutral hydrogen at high redshifts. We used the archival Very Large Telescope (VLT)…

Astrophysics of Galaxies · Physics 2018-08-15 Waqas Bashir , Tayyaba Zafar , Fazeel M. Khan , Farrukh Chishtie

We report the detection of redshifted HI~21cm absorption in the $z \sim 2.347$ damped Lyman-$\alpha$ absorber (DLA) towards PKS B0438-436, with the Green Bank Telescope. This is the second-highest redshift at which 21cm absorption has been…

Astrophysics · Physics 2009-11-11 N. Kanekar , R. Subrahmanyan , S. L. Ellison , W. M. Lane , J. N. Chengalur

We present optical spectra of QSO HS~1946+7658 with either high resolution (FWHM=10 km/s) or high signal to noise ratio (SNR=40-100). We find 113 Lyman alpha and six metal line systems. The metal systems at Zabs=2.844 and 3.050 have complex…

Astrophysics · Physics 2010-12-16 X. -M. Fan , D. Tytler

In order to investigate the physical relationship between strong Ly-alpha absorbers (logN_HI>20.0 cm^-2) such as damped Ly-alpha absorption systems (DLAs) and young star-forming galaxies at high redshift, we have conducted narrow-band…

We present very deep WFPC2 images and FOS spectroscopy from the Hubble Space Telescope (HST) together with numerous supporting ground-based observations of the field of the quasar 3C 336 ($z_{em}=0.927$). The observations are designed to…

Astrophysics · Physics 2016-08-30 C. Steidel , M. Dickinson , D. Meyer , K. Adelberger , K. Sembach

We present results from an ongoing search for galaxy counterparts of a subgroup of Quasar Absorption Line Systems called Damped Ly-alpha Absorbers (DLAs). DLAs have several characteristics that make them prime candidates for being the…

Astrophysics · Physics 2007-05-23 J. U. Fynbo , P. Moller , B. Thomsen

We present a new catalog of absprption-line systems identified in the quasar spectra. It contains data on 821 QSOs and 8558 absorption systems comprizing 16139 absorption lines with measured redshifts in the QSO spectra. The catalog…

Astrophysics · Physics 2007-05-23 A. I. Ryabinkov , A. D. Kaminker , D. A. Varshalovich

We report on a 3600 s spectrum of GRB 021004 obtained with the Nordic Optical Telecope on La Palma 10.71 hours after the burst. We identify absorption lines from five systems at redshifts 1.3806, 1.6039, 2.2983, 2.3230, and 2.3292. In…

The Circum-Galactic Medium (CGM) can be probed through the analysis of absorbing systems in the line-of-sight to bright background quasars. We present measurements of the metallicity of a new sample of 15 sub-damped Lyman-$\alpha$ absorbers…

We estimate the optical depth distribution of dust present in absorption systems along the line of sight of high redshift galaxies and the resulting reddening. We characterize the probability distribution of the transmission to a given…

Astrophysics · Physics 2008-11-26 M. Trenti , M. Stiavelli