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相关论文: Relativistic Outflows in two quasars in the Chandr…

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We have observed the Extended Chandra Deep Field South (E-CDF-S) using a mosaic of six deep Very Large Array (VLA) pointings at 1.4GHz. In this paper, we present the survey strategy, description of the observations, and the first data…

天体物理学 · 物理学 2009-11-13 Neal A. Miller , E. B. Fomalont , K. I. Kellermann , V. Mainieri , C. Norman , P. Padovani , P. Rosati , P. Tozzi

We performed spectroscopic observations of the small-separation lensed quasar SDSS J1001+5027, whose images have an angular separation $\theta \sim 2.^{\!\!\prime\prime}86$, and placed constraints on the physical properties of gas clouds in…

We present the analysis of the absorption troughs of six outflows observed in quasar SDSS J1130+0411 ($z \approx 3.98$) with radial velocities ranging from $-2400$ to $-15,400$ km s$^{-1}$. These spectra were taken with the Very Large…

星系天体物理 · 物理学 2022-09-22 Andrew Walker , Nahum Arav , Doyee Byun

We report the results of two Chandra ACIS-S observations from February and August 2003 of the highly X-ray variable Narrow-Line Seyfert 1 galaxy RX J2217.9--5941. Observations spanning the time from the ROSAT All Sky Survey (RASS) through…

天体物理学 · 物理学 2009-11-10 D. Grupe , K. M. Leighly , V. Burwitz , P. Predehl , S. Mathur

We present results from the deep XMM-Newton observations of the two brightest X-ray sources in the Chandra Deep Field South (CDFS), PID 203 (z=0.544) and PID 319 (z=0.742). The long exposure of 2.5 Ms over a 10 year period (net 4 yr with a…

高能天体物理现象 · 物理学 2015-02-11 K. Iwasawa , C. Vignali , A. Comastri , R. Gilli , F. Vito , W. N. Brandt , F. J. Carrera , G. Lanzuisi , S. Falocco , F. Vagnetti

In the HST/COS spectrum of the Seyfert 1 galaxy 2MASX J14292507+4518318, we have identified a narrow absorption line (NAL) outflow system with a velocity of -151 km s$^{-1}$ This outflow exhibits absorption troughs from the resonance states…

星系天体物理 · 物理学 2023-11-30 Maryam Dehghanian , Nahum Arav , Doyee Byun , Gwen Walker , Mayank Sharma

We analyze VLT/UVES observations of the quasar SDSS J024221.87+004912.6. We identify four absorption outflow systems: a CIV BAL at $v\approx -18,000 \text{ km s}^{-1}$, and three narrower low-ionization systems with centroid velocities…

星系天体物理 · 物理学 2022-03-21 Doyee Byun , Nahum Arav , Patrick B. Hall

We present the first near-infrared interferometric data of a QSO at z=4. The K-band observations were performed with GRAVITY+ on the VLTI using all four UTs, detecting a differential phase signal that traces the spatially resolved…

Quasar redshifts require the best possible precision and accuracy for a number of applications, such as setting the velocity scale for outflows as well as measuring small-scale quasar-quasar clustering. The most reliable redshift standard…

星系天体物理 · 物理学 2017-06-28 Michelle Mason , Michael Brotherton , Adam Myers

We discuss new high-resolution (6.7 km/s) spectra of the associated absorption lines (AALs) in the radio-loud quasar 3C 191. The measured AALs have ionizations ranging from Mg I to N V, and multi-component profiles that are blueshifted by…

天体物理学 · 物理学 2014-10-13 Frederick W. Hamann , T. A. Barlow , F. C. Chaffee , C. B. Foltz , R. J. Weymann

I Zw 1 is the prototype narrow line quasar. We report here the results of our study of the UV emission of I Zw 1 using a high S/N (50-120) spectrum obtained with the HST FOS. The following main new results are obtained: 1. The Mg II and Al…

天体物理学 · 物理学 2009-10-30 Ari Laor , Buell T. Jannuzi , Richard F. Green , Todd A. Boroson

We have observed a sample of 22 luminous quasars, in the range 2.0<z<2.5, at 1.6 microns with the near-infrared (NIR) spectrograph FSPEC on the Multiple Mirror Telescope. Our sample contains 13 radio-loud and 9 radio-quiet objects. We have…

天体物理学 · 物理学 2009-10-31 D. H. McIntosh , H. -W. Rix , M. J. Rieke , C. B. Foltz

We present Subaru observations of the newly discovered luminous quasar AKARI J1757+5907, which shows an absorption outflow in its spectrum. The absorption consists of 9 distinct troughs, and our analysis focuses on the troughs at ~ -1000$…

宇宙学与河外天体物理 · 物理学 2015-05-27 Kentaro Aoki , Shinki Oyabu , Jay P. Dunn , Nahum Arav , Doug Edmonds , Kirk T. Korista , Hideo Matsuhara , Yoshiki Toba

We describe two studies designed to characterize the total column densities, kinetic energies, and acceleration physics of broad absorption line (BAL) outflows in quasars. The first study uses new Chandra X-ray and ground-based rest-frame…

We have investigated a sample of 2099 broad absorption line (BAL) quasars with z=1.7-2.2 built from the Sloan Digital Sky Survey Data Release Seven and the Wide-field Infrared Survey. This sample is collected from two BAL quasar samples in…

星系天体物理 · 物理学 2014-12-24 Shaohua Zhang , Huiyuan Wang , Tinggui Wang , Feijun Xing , Kai Zhang , Hongyan Zhou , Peng Jiang

We report the observation of features near 1 keV in the ASCA spectra from three ``Narrow Line Seyfert 1'' (NLS1) galaxies. We interpret these as oxygen absorption in a highly relativistic outflow. If interpreted as absorption edges, the…

天体物理学 · 物理学 2009-10-30 Karen M. Leighly , Richard F. Mushotzky , Kirpal Nandra , Karl Forster

High velocity (HV) outflows are an important but poorly understood aspect of quasar/SMBH evolution. Outflows during the luminous accretion phase might play a critical role in "unveiling" young dusty AGN and regulating star formation in the…

天体物理学 · 物理学 2007-05-23 Paola Rodriguez Hidalgo , Fred Hamann , Daniel Nestor , Joseph Shields

While stellar processes are believed to be the main source of feedback in dwarf galaxies, the accumulating discoveries of AGN in dwarf galaxies over recent years arouse the interest to also consider AGN feedback in them. Fast, AGN-driven…

We present results from a comprehensive study of ultrafast outflows (UFOs) detected in a sample of fourteen quasars, twelve of which are gravitationally lensed, in a redshift range of 1.41-3.91, near the peak of the AGN and star formation…

In this Paper we present the source catalog obtained from a 942 ks exposure of the Chandra Deep Field South (CDFS), using ACIS-I on the Chandra X-ray Observatory. Catalog generation proceeded simultaneously using two different methods; a…