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相关论文: The Search for Extragalactic Lithium Hydride

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We present an absorption line analysis of the Lyman limit system (LLS) at z=3.55 in our Magellan/MIKE spectrum of PKS2000-330. Our analysis of the Lyman limit and full HI Lyman series constrains the total HI column density of the LLS (N_HI…

宇宙学与河外天体物理 · 物理学 2014-11-20 Gabriel E. Prochter , J. Xavier Prochaska , John M. O'Meara , Scott Burles , Rebecca A. Bernstein

We have analyzed the spectrum of the quasar PKS 1232+082 obtained by Petitjean et al. (2000). HD molecular lines are identified in an absorption system at the redshift z=2.3377. The column density of HD molecules in the system is estimated,…

天体物理学 · 物理学 2009-11-06 D. Varshalovich , A. Ivanchik , P. Petitjean , R. Srianand , C. Ledoux

We present a novel method to investigate cosmic reionization, using joint spectral information on high redshift Lyman Alpha Emitters (LAE) and quasars (QSOs). Although LAEs have been proposed as reionization probes, their use is hampered by…

宇宙学与河外天体物理 · 物理学 2015-06-04 S. Baek , A. Ferrara , B. Semelin

We present the results of XMM-Newton observations of four high-z quasars, two radio-loud and two radio-quiet. One of the radio-loud objects, PKS 2126-158, clearly shows absorption in excess of the galactic value as claimed before from ASCA…

天体物理学 · 物理学 2011-05-23 E. Ferrero , W. Brinkmann

We report the discovery of a galaxy at a redshift z = 6.17 identified from deep narrow band imaging and spectroscopic follow-up in one of the CFHT-VIRMOS deep survey fields at 0226-04. In addition to the existing deep BVRI images of this…

天体物理学 · 物理学 2011-05-23 J. -G. Cuby , O. Le Fevre , H. McCracken , J. -C. Cuillandre , E. Magnier , B. Meneux

We present the results of ground-based and HST imaging studies targeted on z>4.5 quasar fields. High-redshift galaxies identified in deep narrow-band Lyman alpha images of the fields surrounding the quasars BR1202-0725 (z=4.694) and…

天体物理学 · 物理学 2007-05-23 Esther M. Hu , Richard G. McMahon , Eiichi Egami

We present a study of the galaxy environment of 9 strong HI+CIV absorption line systems ($16.2<{\rm log}(N({\rm HI}))<21.2$) spanning a wide range in metallicity at $z\sim4-5$, using MUSE integral field and X-Shooter spectroscopic data…

We present an absorption-line survey of optically thick gas clouds -- Lyman Limit Systems (LLSs) -- observed at high dispersion with spectrometers on the Keck and Magellan telescopes. We measure column densities of neutral hydrogen NHI and…

宇宙学与河外天体物理 · 物理学 2015-10-14 J. Xavier Prochaska , John M. O'Meara , Michele Fumagalli , Rebecca A. Bernstein , Scott M. Burles

We report the detection of a third HI 21-cm absorber in the sight-line towards the z=2.64 quasar MG J0414+0534 (4C +05.19). In addition to the absorption at the host redshift and in the z=0.96 gravitational lens, we find, through a…

宇宙学与河外天体物理 · 物理学 2015-05-27 S. J. Curran , M. T. Whiting , A. Tanna , C. Bignell , J. K. Webb

We report observations of four sub-damped Lyman-alpha (sub-DLA) quasar absorbers at z<0.5 obtained with the Hubble Space Telescope Cosmic Origins Spectrograph. We measure the available neutrals or ions of C, N, O, Si, P, S, Ar, Mn, Fe,…

宇宙学与河外天体物理 · 物理学 2015-06-11 Debopam Som , Varsha P. Kulkarni , Joseph Meiring , Donald G. York , Celine Péroux , James T. Lauroesch , Monique C. Aller , Pushpa Khare

We have used the Taurus Tunable Filter to search for Lyman alpha emitters in the fields of three high redshift quasar fields: two at z~2.2 (MRC B1256-243 and MRC B2158-206) and one at z~4.5 (BR B0019-1522). Our observations had a field of…

宇宙学与河外天体物理 · 物理学 2012-05-23 John Swinbank , Joanne Baker , Jordi Barr , Isobel Hook , Joss Bland-Hawthorn

We report the discovery of a new double-image quasar that was found during a search for gravitational lenses in the southern sky. Radio source PMN J1838-3427 is composed of two flat-spectrum components with separation 1", flux density ratio…

As part of a program to study the relationship between QSO Lyman alpha clouds and galaxies at low redshifts, we have obtained a high signal-to-noise far UV spectrum of H 1821+643 [z(em) = 0.297] with the G140L grating of the GHRS. The…

天体物理学 · 物理学 2007-05-23 T. M. Tripp , L. Lu , B. D. Savage

We examine the Ly-alpha absorber population at z<0.3 detected in spectra of the QSOs PG0953+415 and H1821+643 taken with the Space Telescope Imaging Spectrograph aboard the Hubble Space Telescope. We compare their statistical properties to…

天体物理学 · 物理学 2009-11-06 Romeel Davé , Todd M. Tripp

We present observations of SDSSp J104433.04--012502.2, a luminous quasar at z=5.80 discovered from Sloan Digital Sky Survey (SDSS) multicolor imaging data. This object was selected as an i'-band dropout object, with i*=21.8 +/- 0.2, z*=19.2…

We present HST/WFPC2 broadband and ground-based Halpha images, H I 21-cm emission maps, and low-resolution optical spectra of the nearby galaxy ESO 1327-2041, which is located 38 arcsec (14 kpc in projection) west of the quasar PKS…

宇宙学与河外天体物理 · 物理学 2012-06-15 B. A. Keeney , J. T. Stocke , C. W. Danforth , C. L. Carilli

We present a method for studying the proximity effect and the density structure around redshift z=2-3 quasars. It is based on the probability distribution of Lyman-alpha pixel optical depths and its evolution with redshift. We validate the…

天体物理学 · 物理学 2016-08-30 E. Rollinde , R. Srianand , T. Theuns , P. Petitjean , H. Chand

We examine the properties of two galaxy "halos" at z ~ 0.7 in the TON 153 (z_em = 1.01) quasar field. The first absorber-galaxy pair (G1) is a z = 0.672, L_B = 4.3 L*_B, E/S0 galaxy probed at D = 58 kpc. G1 is associated with a remarkable…

天体物理学 · 物理学 2011-02-11 Christopher W. Churchill , Glenn G. Kacprzak , Charles C. Steidel , Jessica L. Evans

We present the results of a survey for damped (DLA, log N(H I) > 20.3) and sub-damped Lyman-? systems (19.5 < log N(H I) < 20.3) at z > 2.55 along the lines-of-sight to 77 quasars with emission redshifts in the range 4 < zem < 6.3.…

Using VLT/X-shooter we searched for emission line galaxies associated to four damped Lyman-$\alpha$ systems (DLAs) and one sub-DLA at 2.73<=z<=3.25 towards QSO J2358+0149. We detect [O III] emission from a "low-cool" DLA at z_abs = 2.9791…

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