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With close pairs of quasars at different redshifts, a background quasar sightline can be used to study a foreground quasar's environment in absorption. We search 149 moderate resolution background quasar spectra, from Gemini, Keck, the MMT,…

We report the GMRT detection of HI 21cm absorption from the $z \sim 3.39$ damped Lyman-$\alpha$ absorber (DLA) towards PKS 0201+113, the highest redshift at which 21cm absorption has been detected in a DLA. The absorption is spread over…

Astrophysics · Physics 2008-11-26 N. Kanekar , J. N. Chengalur , W. M. Lane

Damped Lyman-alpha systems (DLAs) and sub-DLAs seen toward background quasars provide the most detailed probes of elemental abundances. Somewhat paradoxically these measurements are more difficult at lower redshifts due to the atmospheric…

Astrophysics · Physics 2009-11-13 C. Peroux , J. D. Meiring , V. P. Kulkarni , P. Khare , J. T. Lauroesch , G. Vladilo , D. G. York

Eleven candidate damped Lya absorption systems were identified in 27 spectra of the quasars from the APM z>4 survey covering the redshift range 2.8<z(abs)<4.4 (8 with z(abs)>3.5). High resolution echelle spectra (0.8A FWHM) have been…

Astrophysics · Physics 2015-06-24 L. J. Storrie-Lombardi , M. J. Irwin , R. G. McMahon

SDSS J095253.83+011422.0 (SDSS J0952+0114) was reported by Hall et al. (2004) as an exotic quasar at $z_{\rm em}=3.020$. In contrast to prominent broad metal--line emissions with FWHM~9000 km/s, only a narrow Ly \alpha emission line is…

We interpret observations of intergalactic low ionisation metal absorption systems at redshifts z $\gtrsim$5 in terms of pressure-confined clouds. We find clouds confined by the expected pressure of galactic haloes with masses $11<\log…

Cosmology and Nongalactic Astrophysics · Physics 2021-01-27 Teresita Suarez , Avery Meiksin

Proximate molecular quasar absorbers (PH2) are an intriguing population of absorption systems recently uncovered through strong H2 absorption at small velocity separation from the background quasars. We performed a multi-wavelength…

Astrophysics of Galaxies · Physics 2023-05-10 P. Noterdaeme , S. Balashev , R. Cuellar , J. -K. Krogager , F. Combes , A. De Cia , N. Gupta , C. Ledoux , S. López , R. Srianand

We used the photometric database of the Sloan Digital Sky Survey (SDSS) to estimate the reddening of 13 SDSS quasars selected on the basis of the presence of zinc absorption lines in an intervening Damped Ly alpha (DLA) system. In 5 of…

Astrophysics · Physics 2008-11-26 G. Vladilo , M. Centurion , S. A. Levshakov , C. Peroux , P. Khare , V. P. Kulkarni , D. G. York

We measure the effect of high column density absorbing systems of neutral hydrogen (HI) on the one-dimensional (1D) Lyman-alpha forest flux power spectrum using cosmological hydrodynamical simulations from the Illustris project. High column…

Cosmology and Nongalactic Astrophysics · Physics 2018-01-10 Keir K. Rogers , Simeon Bird , Hiranya V. Peiris , Andrew Pontzen , Andreu Font-Ribera , Boris Leistedt

The goal of the Complete Optical and Radio Absorption Line System (CORALS) survey is to quantify the potential impact on QSO absorber statistics from dust in intervening galaxies. Dust may introduce a selection bias in surveys which are…

Astrophysics · Physics 2009-11-10 Sara L. Ellison , Chris W. Churchill , Samantha A. Rix , Max Pettini

We present the detection of the average H$_2$ absorption signal in the overall population of neutral gas absorption systems at $z\sim 3$ using composite absorption spectra built from the Sloan Digital Sky Survey-III damped Lyman-$\alpha$…

Astrophysics of Galaxies · Physics 2018-05-02 Sergei Balashev , Pasquier Noterdaeme

Study of Lyman-alpha absorption lines in the spectra of double line of sight (DLOS) quasars holds the promise of diagnosing the nature of the structures that give rise to Lyman-alpha absorption. Based on simulations of DLOS with various…

Astrophysics · Physics 2009-10-28 Jane C. Charlton , Christopher W. Churchill , Suzanne M. Linder

We present results for QSO PKS 0405-123 (z=0.574, V=14.9), as part of a STIS Investigation Definition Team (IDT) key project to study weak Ly-alpha forest systems at low z. We detect 59 (47) Ly-alpha absorbers at 4.0 sigma significance to…

Astrophysics · Physics 2007-05-23 G. Williger , S. Heap , R. Weymann , R. Dave , T. Tripp

We present a sample of 33 damped Lyman alpha systems (DLAs) discovered in the Sloan Digital Sky Survey (SDSS) whose absorption redshifts (z_abs) are within 6000 km/s of the QSO's systemic redshift (z_sys). Our sample is based on 731 2.5 <…

Astrophysics · Physics 2009-11-13 David M. Russell , Sara L. Ellison , Chris R. Benn

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

We present a new ultra-violet spectrum of the QSO 0013-004 with 0.9 \AA resolution obtained with the MMT Blue spectrograph. The \upsilon = 0 - 0, 1 - 0, 2 - 0 and 3 - 0 Lyman bands of H_2 associated with the z = 1.9731 damped Ly alpah…

Astrophysics · Physics 2016-08-30 Jian Ge , Jill Bechtold

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 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 have conducted a long slit search for low surface brightness Lyman-alpha emitters at redshift 2.67 < z < 3.75. A 92 hour long exposure with VLT/FORS2 down to a 1-sigma surface brightness detection limit of 8x10^-20 erg/cm2/s/sqarcsec…

In this paper, we present an intercomparison study of two quasars, SDSS J145618.32+340037.2 and SDSS J215331.50-025514.1, which have proximate damped Lya systems (PDLAs) with residual flux upon the Lya absorption trough. Though they both…

Astrophysics of Galaxies · Physics 2018-05-16 Xiaoyi Xie , Hongyan Zhou , Xiang Pan , Peng Jiang , Xiheng Shi , Tuo Ji , Shaohua Zhang , Shengmiao Wu , Zhihao Zhong
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