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Related papers: A Quasar Without Broad Lyman-alpha Emission

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The radio-quiet quasar SDSS J1240+1455 lies at a redshift of z=3.11, is surrounded by a Ly-alpha blob (LAB), and is absorbed by a proximate damped Ly-alpha system. In order to better define the morphology of the blob and determine its…

Astrophysics of Galaxies · Physics 2024-02-14 P. North , M. Hayes , M. Millon , A. Verhamme , M. Trebitsch , J. Blaizot , F. Courbin , D. Chelouche

We present spectra taken with the Low Resolution Imaging Spectrograph on the Keck 10m telescope of spatially-resolved structures ("fuzz") around the high-redshift radio-loud quasars PKS 0445+097 (z=2.108) and PKS 2338+042 (z=2.589). For PKS…

Astrophysics · Physics 2007-05-23 Matthew D. Lehnert , Robert H. Becker

Based on 5344 quasar spectra taken from the SDSS Data Release 2, the dependences of various emission-line flux ratios on redshift and quasar luminosity are investigated in the ranges 2.0 < z < 4.5 and -24.5 > M_B > -29.5$. We show that the…

Astrophysics · Physics 2009-11-11 Tohru Nagao , Alessandro Marconi , Roberto Maiolino

We have obtained quasi-simultaneous ultraviolet-optical spectra for 22 out of 23 quasars in the complete PG-X-ray sample with redshift, z<0.4, and M_B<-23. The spectra cover rest-frame wavelengths from at least Lyman-alpha to H-alpha. Here…

Astrophysics · Physics 2008-11-26 Zhaohui Shang , Beverley J. Wills , D. Wills , Michael S. Brotherton

Comparison of six high-redshift quasar spectra obtained with the Large Binocular Telescope with previous observations from the Sloan Digital Sky Survey shows that failure to correctly identify absorption and other problems with accurate…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-15 Kelly D. Denney , Richard W. Pogge , Roberto J. Assef , Christopher S. Kochanek , Bradley M. Peterson , Marianne Vestergaard

We present a detailed study of the optical and NIR emission and absorption line spectrum of the quasar SDSS J163345.22+512748.4. We discovered on the newly acquired NIR spectrum a highly meta-stable neutral helium broad absorption line…

Astrophysics of Galaxies · Physics 2022-04-01 Bo Liu , Hongyan Zhou , Xinwen Shu , Shaohua Zhang , Tuo Ji , Xiang Pan , Peng Jiang

We report the archival discovery of Lyman-$\alpha$ emission from the bright ultraviolet galaxy Y002 at $z=7.677$, spectroscopically confirmed by its ionized carbon [CII] 158$\mu$m emission line. The Ly$\alpha$ line is spatially associated…

We report the discovery of superstrong, fading, high-ionization iron line emission in the galaxy SDSSJ095209.56+214313.3 (SDSSJ0952+2143 hereafter), which must have been caused by an X-ray outburst of large amplitude. SDSSJ0952+2143 is…

Astrophysics · Physics 2010-11-11 S. Komossa , H. Zhou , T. Wang , M. Ajello , J. Ge , J. Greiner , H. Lu , M. Salvato , R. Saxton , H. Shan , D. Xu , W. Yuan

We present deep Keck/MOSFIRE near-infrared spectroscopy of a strong Lyman alpha emitting source at z=6.1292, HSC J142331.71-001809.1, which was discovered by the SHELLQS program from imaging data of the Subaru Hyper Suprime-Cam (HSC)…

We searched for star formation activity associated with high-z Damped Lyman-alpha systems (DLAs) with Subaru telescope. We used a set of narrow-band (NB) filters whose central wavelengths correspond to the redshifted Lyman-alpha emission…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-18 Nobunari Kashikawa , Toru Misawa , Yosuke Minowa , Katsuya Okoshi , Takashi Hattori , Jun Toshikawa , Shogo Ishikawa , Masafusa Onoue

We report the serendipitous discovery of two objects close in projection with fairly strong emission lines at long wavelength (~9190 A). One (A) seems not to be hosted by any galaxy brighter than V(555)=27.5, or I(814)=26.7 (Vega-based…

Astrophysics · Physics 2009-10-31 Daniel Stern , Andrew J. Bunker , Hyron Spinrad , Arjun Dey

We present a detailed analysis of chemical abundances in a sub-damped Lyman alpha absorber at z=1.839 towards the quasar B1101-26, based on a very-high-resolution (R ~ 75,000) and high-signal-to-noise (S/N >100) spectrum observed with the…

Astrophysics of Galaxies · Physics 2014-12-10 Anne Fox , Philipp Richter , Cora Fechner

The number of damped Ly-alpha absorbers (DLAs) currently known is about 100, but our knowledge of their sizes and morphologies is still very sparse as very few have been detected in emission. Here we present narrow-band and broad-band…

Astrophysics · Physics 2016-08-30 J. U. Fynbo , P. Moller , S. J. Warren

We report optical Cousins R and I band monitoring observations of the high redshift (z = 4.67) QSO SDSS J153259.96-003944.1 that does not show detectable emission lines in its optical spectrum. We show this object varies with a maximum…

Astrophysics · Physics 2009-11-10 C. S. Stalin , R. Srianand

We report the discovery of rapid variations of a high-velocity CIV broad absorption line trough in the quasar SDSS J141007.74+541203.3. This object was intensively observed in 2014 as a part of the Sloan Digital Sky Survey Reverberation…

We present a total of 4784 unique broad absorption line quasars from the Sloan Digital Sky Survey Third Data Release. An automated algorithm was used to match a continuum to each quasar and to identify regions of flux at least 10% below the…

We report the results from an ASCA observation of the high-luminosity, radio-loud quasar PKS 0637-752 (redshift 0.654), covering the 0.8-15 keV band in the quasar-frame. We find the source to have a luminosity ~10^46 erg/s in the 2-10 keV…

Astrophysics · Physics 2009-10-30 T. Yaqoob , I. M. George , T. J. Turner , K. Nandra , A. Ptak , P. J. Serlemitsos

We report the serendipitous discoveries of companion galaxies to two high-redshift quasars. SDSS J025617.7+001904 is a z=4.79 quasar included in our recent survey of faint quasars in the SDSS Stripe 82 region. The initial MMT slit…

We report on the highly variable SiIV and CIV broad absorption lines in SDSS J113831.4+351725.2 across four observational epochs. Using the SiIV doublet components, we find that the blue component is usually saturated and non-black, with…

Astrophysics of Galaxies · Physics 2015-03-03 Conor Wildy , Michael R. Goad , James T. Allen

We present evidence that the high-velocity CIV lambda 1549 emission line gas of radio-loud quasars may originate in a disk-like configuration, in close proximity to the accretion disk often assumed to emit the low-ionization lines. For a…

Astrophysics · Physics 2009-10-31 M. Vestergaard , B. J. Wilkes , P. D. Barthel