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相关论文: The Origins of a Rich Absorption Line Complex in a…

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We present further results of a survey for absorption line systems in the spectra of four high redshift quasars (5.79 $\le$ z$_{\textrm{em}}$ $\le$ 6.13) obtained with the ESO Very Large Telescope X-Shooter. We identify 36 $\textrm{CIV}$…

Quasar spectra have a variety of absorption lines whose origins range from energetic winds expelled from the central engines to unrelated, intergalactic clouds. We present multi-epoch, medium resolution spectra of eight quasars at z~2 that…

天体物理学 · 物理学 2009-11-10 Desika Narayanan , Fred Hamann , Tom Barlow , E. M. Burbidge , Ross D. Cohen , Vesa Junkkarinen , Ron Lyons

To investigate the evolution of metal-enriched gas over recent cosmic epochs as well as to characterize the diffuse, ionized, metal-enriched circumgalactic medium (CGM), we have conducted a blind survey for C IV absorption systems in 89 QSO…

We report the discovery of an unambiguous, substantial low-energy cutoff in the broad band X-ray spectrum of the radio quasar RXJ1028.6-0844 at a redshift of 4.276 obtained with the ASCA satellite, which we preferably explained as…

天体物理学 · 物理学 2009-10-31 W. Yuan , M. Matsuoka , T. Wang , S. Ueno , H. Kubo , T. Mihara

The physical conditions of the circumgalactic medium are probed by intervening absorption-line systems in the spectrum of background quasi-stellar objects out to the epoch of cosmic reionization. A correlation between the ionization state…

We examine the relationship between galaxies and the intergalactic medium at z < 1 using a group of three closely spaced background QSOs with z_em ~1 observed with the Hubble Space Telescope. Using a new grouping algorithm, we identify…

宇宙学与河外天体物理 · 物理学 2015-05-14 Neil H. M. Crighton , Simon L. Morris , Jill Bechtold , Robert A. Crain , Buell T. Jannuzi , Allen Shone , Tom Theuns

We present a sample of 46 [OIII]-emitting galaxies at z<0.8 detected in the fibre spectra of quasars from the SDSS-DR7 through an automatic search procedure. We also detect [OII] and Hb emission lines from most of these galaxies in the SDSS…

宇宙学与河外天体物理 · 物理学 2015-05-14 P. Noterdaeme , R. Srianand , V. Mohan

We present the analysis of two outflows (S1 at --5500 km s$^{-1}$ and S2 at --9700 km s$^{-1}$) seen in recent HST/COS observations of quasar SDSS J0755+2306 (z = 0.854). The outflows are detected as absorption troughs from both…

星系天体物理 · 物理学 2020-03-25 Xinfeng Xu , Nahum Arav , Timothy Miller , Gerard A. Kriss , Rachel Plesha

We list and analyze H I absorption lines at redshifts 2 < z < 4 with column density (12 < log(N_HI) < 19) in 40 high-resolutional (FWHM = 8.0 km/s) quasar spectra obtained with the Keck+HIRES. We de-blend and fit all H I lines within 1,000…

天体物理学 · 物理学 2008-11-26 T. Misawa , D. Tytler , M. Iye , D. Kirkman , N. Suzuki , D. Lubin , N. Kashikawa

We report on the multiphase absorption-line system detected at a redshift z = 3.021 in the spectrum of the quasi-stellar object CTQ 325 (z_em = 3.212). The system is displaced by ~14,000 km/s to the blue of the systemic velocity defined by…

天体物理学 · 物理学 2009-11-10 S. A. Levshakov , S. D'Odorico , I. I. Agafonova , M. Dessauge-Zavadsky

We present images and spectroscopy of objects close to the sightline of Q2302+029 in order to search for galaxies responsible for the remarkable z=0.7 high-ionization absorption line system found by Jannuzi et al (1996). This system shows…

天体物理学 · 物理学 2009-10-31 David V. Bowen , Raul Jimenez , Edward B. Jenkins , Max Pettini

We present results from 12 km/s resolution echelle spectroscopy of the bright $z=4.694$ QSO BR1202-0725. A preliminary analysis shows that high metallicity narrow line absorption clouds are present up to the redshift of the quasar. A damped…

天体物理学 · 物理学 2007-05-23 E. J. Wampler , G. M. Williger , J. A. Baldwin , R. F. Carswell , C. Hazard , R. G. McMahon

We present a new spectrum of the quasar HS1603+3820 taken 1.28 years (0.36 years in the quasar rest frame) after a previous observation with Subaru+HDS. The new spectrum enables us to search for time variability as an identifier of…

天体物理学 · 物理学 2009-11-11 Toru Misawa , Michael Eracleous , Jane C. Charlton , Akito Tajitsu

We report a serendipitous discovery of broad absorption lines that were newly formed in the spectrum of the high-redshift, luminous radio-loud quasar TEX 1726 + 344, in a time interval of only 12 years. This is the first quasar showing a…

天体物理学 · 物理学 2009-11-07 Feng Ma

SDSS J072910.34+333634.3 is a reddened quasar at z=0.96. The archivel Keck/ESI spectrum and our new P200/TripleSpec spectrum reveal an absorption line system in He I*, Ca II H\&K and Na ID. The absorption line system has a width of…

星系天体物理 · 物理学 2016-12-19 Tong Liu , Luming Sun , Xiang Pan , Hongyan Zhou

An analysis of ~19500 narrow (<200 km/s) CIV 1548.2,1550.8 absorbers in ~34000 Sloan Digital Sky Survey quasar spectra is presented. The statistics of the number of absorbers as a function of outflow-velocity shows that in approximately…

星系天体物理 · 物理学 2015-06-22 Rebecca A. A. Bowler , Paul C. Hewett , James T. Allen , Gary J. Ferland

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…

天体物理学 · 物理学 2007-05-23 A. I. Ryabinkov , A. D. Kaminker , D. A. Varshalovich

In the course of a large intervening MgII survey of 25 quasars, the CIV emission lines of six (three radio-loud and three radio-quiet) were observed serendipitously. In four of these six quasars, we detected associated narrow absorption…

天体物理学 · 物理学 2007-05-23 Rajib Ganguly , Michael Eracleous , Jane C. Charlton , Christopher W. Churchill

We present analysis on three intervening H I-C IV absorption systems tracing gas within galaxy group/cluster environments, identified in the $HST$/COS far-UV spectra of the background quasars PG $1148+549$ ($z_{abs}=0.00346$),…

星系天体物理 · 物理学 2019-03-12 Aditya Manuwal , Anand Narayanan , Sowgat Muzahid , Jane C. Charlton , Vikram Khaire , Hum Chand

We consider geometries and possible physical models for weak low ionization absorbers based on the relative incidence of low and high ionization absorption systems. We found a total of 16 metal-line systems, with low and/or high ionization…