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相关论文: Dust Biasing of Damped Lyman Alpha Systems: a Baye…

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We investigate the population of z=3 damped Lyman alpha absorbers (DLAs) in a recent series of high resolution galaxy formation simulations. The simulations are of interest because they form at z=0 some of the most realistic disk galaxies…

We study the dust depletion pattern in eight well separated components of the z=1.973, logN(HI)=20.83, damped Lyman-alpha system toward Q0013-004, four of which have detectable H2 absorption. The apparent correlation between the abundance…

天体物理学 · 物理学 2009-11-07 Patrick Petitjean , R. Srianand , Cédric Ledoux

Interpreting abundances of Damped Ly-$\alpha$ Absorbers (DLAs) from absorption-line spectroscopy has typically been a challenge because of the presence of dust. Nevertheless, because DLAs trace distant gas-rich galaxies regardless of their…

星系天体物理 · 物理学 2018-04-04 Annalisa De Cia , Cédric Ledoux , Patrick Petitjean , Sandra Savaglio

We present HST spectra for a sample of six QSOs with intermediate redshift (z_a < 1) damped Ly-alpha systems. These observations aim at measuring the HI column density and detect metal lines in order to investigate the metal enrichment of…

天体物理学 · 物理学 2007-05-23 Patrick Boisse , Vincent Le Brun , Jacqueline Bergeron , Jean-Michel Deharveng

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…

We present 4 new measurements of nitrogen abundances and one upper limit in damped Lyman alpha absorbers (DLAs) obtained by means of high resolution (FWHM \~ 7 km/s) UVES/VLT spectra. In addition to these measurements we have compiled data…

天体物理学 · 物理学 2011-05-23 M. Centurion , P. Molaro , G. Vladilo , C. Peroux , S. A. Levshakov , V. D'Odorico

We present a new sample of 31 CaII(H&K) 3935,3970 absorption line systems with 0.84<z_abs<1.3 discovered in the spectra of Sloan Digital Sky Survey (SDSS) Data Release 3 quasars, together with an analysis of their dust content. The presence…

天体物理学 · 物理学 2009-11-11 Vivienne Wild , Paul C. Hewett

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.…

天体物理学 · 物理学 2016-01-27 Jayaram N. Chengalur , A. G. de Bruyn , R. Braun , C. L. Carilli

Damped Lyman-$\alpha$ absorbers (DLAs) with molecular hydrogen have been probed in detail through both spectroscopic observations and numerical modelling. However, such H$_2$ absorbers are quite sparse at very high redshifts. We identify…

星系天体物理 · 物理学 2025-03-20 Aashiya Anitha Shaji , Katherine Rawlins , Pranshu Kurel

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

We present results from a search for galaxies that give rise to damped Lyman alpha (DLA), subDLA, and Lyman limit system (LLS) absorption at redshifts 0.1 ~< z ~< 1 in the spectra of background quasars. The sample was formed from a larger…

宇宙学与河外天体物理 · 物理学 2015-05-27 Sandhya M. Rao , Michele Belfort-Mihalyi , David A. Turnshek , Eric M. Monier , Daniel B. Nestor , Anna M. Quider

In this paper we point out a previously unnoticed anticorrelation between the observed abundance ratio [X/Zn] (where Zn is assumed to be undepleted and X stands for the refractories Fe, Cr and Ni) and metal column density…

天体物理学 · 物理学 2009-11-06 J. L. Hou , S. Boissier , N. Prantzos

Radio-selected samples of quasars with complete optical identifications offer an ideal dataset with which to investigate dust bias associated with intervening absorption systems. Here, we review our work on the Complete Optical and Radio…

天体物理学 · 物理学 2009-11-11 Sara L. Ellison

We study the H2 molecular content in high redshift damped Lyman-alpha systems (DLAs) as a function of the HI column density. We find a significant increase of the H2 molecular content around log N(HI) (cm^-2)~21.5-22, a regime unprobed…

宇宙学与河外天体物理 · 物理学 2015-06-10 P. Noterdaeme , P. Petitjean , R. Srianand

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…

We use simple models of the spatial structure of the quasar broad line region (BLR) to investigate the properties of so-called ghostly damped Lyman-{\alpha} (DLA) systems detected in SDSS data. These absorbers are characterized by the…

星系天体物理 · 物理学 2021-02-03 Brivael Laloux , Patrick Petitjean , Camille Noûs

Using a spectral stacking technique we searched for the average \lya emission from high-z Damped \lya (DLA) galaxies detected in the Sloan Digital Sky Survey QSO spectra. We used a sample of 341 DLAs of mean redshift <z>= 2.86 and log N(HI)…

宇宙学与河外天体物理 · 物理学 2015-05-19 H. Rahmani , R. Srianand , P. Noterdaeme , P. Petitjean

The damped Lyman alpha absorbers (DLAs) in quasar spectra are believed to be the progenitors of present-day disk galaxies. We examine the probability for microlensing of background quasars by stars in their DLAs. Microlensing by an…

天体物理学 · 物理学 2009-10-30 Rosalba Perna , Abraham Loeb

The Baryon Oscillation Spectroscopic Survey of SDSS-III has provided an unprecedentedly large sample of Damped \lya systems (DLAs), the largest repositories of neutral hydrogen in the Universe. This DLA sample has been used to determine the…

(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…