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Spectroscopy of QSO absorption lines provides essential observational input for the study of nucleosynthesis and chemical evolution of galaxies at high redshift. But new observations may indicate that present chemical abundance data are…

天体物理学 · 物理学 2007-05-23 R. Quast , D. Reimers , A. Smette , O. Garcet , C. Ledoux , S. Lopez , L. Wisotzki

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,…

天体物理学 · 物理学 2009-11-10 Celine Peroux , Jean-Michel Deharveng , Vincent Le Brun , Stefano Cristiani

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 essential in the process of…

天体物理学 · 物理学 2007-05-23 J. U. Fynbo , B. Thomsen , P. Moller

We have carried out a high angular resolution near-infrared imaging study of the fields of 6 quasars with 7 strong absorption line systems at z < 0.5, using the Hokupa'a adaptive optics system and the QUIRC near-infrared camera on the…

天体物理学 · 物理学 2008-11-26 Mark R. Chun , Soheila Gharanfoli , Varsha P. Kulkarni , Marianne Takamiya

We report on a sensitive search for redshifted H$\alpha$ line-emission from three high-metallicity damped Ly$\alpha$ absorbers (DLAs) at $z \approx 2.4$ with the Near-infrared Integral Field Spectrometer (NIFS) on the Gemini-North…

星系天体物理 · 物理学 2015-06-23 Wei-Hao Wang , Nissim Kanekar , J. Xavier Prochaska

We report on further observations of the field of the quasar Q1218+0832. Geier et al. 2019 presented the discovery of the quasar resulting from a search for quasars reddened and dimmed by dust in foreground damped Lyman-alpha absorbers…

Damped Lyman-alpha absorbers (DLAs), seen in absorption against a background quasar, provide the most detailed probes available of element abundances in the Universe over > 90 % of its age. DLAs can be used to observationally measure the…

天体物理学 · 物理学 2009-11-11 C. Peroux , J. D. Meiring , V. P. Kulkarni , R. Ferlet , P. Khare , J. T. Lauroesch , G. Vladilo , D. G. York

We compare the properties of a sample of local (z=0) gas-rich galaxies studied in 21 cm emission to a sample of 13 low-redshift (z < 1) damped Lyman alpha (DLA) galaxies identified as the counterparts of low-redshift DLA systems found in…

天体物理学 · 物理学 2007-05-23 David A. Turnshek , Sandhya M. Rao , Daniel B. Nestor

We use the average E(B-V) and ZnII column densities of a sample of z~1 CaII (3935, 3970) absorption line systems selected from the Sloan Digital Sky Survey (SDSS DR4) to show that on average, with conservative assumptions regarding…

天体物理学 · 物理学 2009-11-11 Vivienne Wild , Paul Hewett , Max Pettini

In this paper we investigate the possible reasons why HI 21-cm absorption in damped Lyman-alpha systems (DLAs) has only been detected at low redshift... We suggest that the lack of 21-cm absorption detections at high redshift arises from…

天体物理学 · 物理学 2009-11-11 S. J. Curran , J. K. Webb

We present high resolution echelle spectra of 7 proximate damped Lyman alpha (PDLA) systems whose relative velocity separation from the background quasar is Delta V < 3000 km/s. Combining our sample with a further 9 PDLAs from the…

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 present results of our HST Cycle 11 Survey for low-redshift (z<1.65) DLAs in the UV spectra of quasars selected from the SDSS Early Data Release. These quasars have strong intervening MgII-FeII systems which are known signatures of high…

天体物理学 · 物理学 2009-11-13 Sandhya M. Rao , David A. Turnshek , Daniel. B. Nestor

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…

We have obtained very deep near-infrared images in the fields of 10 QSOs whose spectra contain damped Lyman-alpha absorption (DLA) systems with 1.7<z_abs <2.5. The main aim of our investigation is to provide new constraints on the…

天体物理学 · 物理学 2015-06-24 A. Aragon-Salamanca , R. S. Ellis , K. S. O'Brien

We report the discovery of a "super-damped" Lyman-alpha absorber at $z_{abs}=2.2068$ toward QSO Q1135-0010 in the Sloan Digital Sky Survey, and follow-up VLT UVES spectroscopy. Voigt profile fit to the DLA line indicates log $N_{\rm H I} =…

宇宙学与河外天体物理 · 物理学 2012-02-23 Varsha P. Kulkarni , Joseph Meiring , Debopam Som , Celine Peroux , Donald G. York , Pushpa Khare , James T. Lauroesch

Starting from a summary of detection statistics of our recent X-shooter campaign, we review the major surveys, both space and ground based, for emission counterparts of high-redshift damped Ly$\alpha$ absorbers (DLAs) carried out since the…

星系天体物理 · 物理学 2017-06-19 Jens-Kristian Krogager , Palle Møller , Johan P. U. Fynbo , Pasquier Noterdaeme

(Abridged for arXiv) We report the discovery of an unusual, extremely dust-rich and metal-strong damped \lya absorption system (DLA) at a redshift $z_{a}=2.4596$ toward the quasar SDSS J115705.52+615521.7 (hereafter J1157+6155) with an…

We cross-correlate the positions of damped Lyman-$\alpha$ systems (DLAs) and their parent quasar catalog with a convergence map derived from the Planck cosmic microwave background (CMB) temperature data. We make consistent measurements of…

宇宙学与河外天体物理 · 物理学 2020-08-27 David Alonso , Joseph Colosimo , Andreu Font-Ribera , Anže Slosar

We present a study of ~100 high redshift (z~2-4) extremely strong damped Lyman-alpha systems (ESDLA, with N(HI)>0.5x10^22 cm^-2) detected in quasar spectra from the Baryon Oscillation Spectroscopic Survey SDSS-III DR11. We study the neutral…

星系天体物理 · 物理学 2014-07-01 P. Noterdaeme , P. Petitjean , I. Paris , Z. Cai , H. Finley , J. Ge , M. M. Pieri , D. G. York