Results 51 to 60 of about 111,241 (293)
Improved redshifts for SDSS quasar spectra [PDF]
A systematic investigation of the relationship between different redshift estimation schemes for more than 91000 quasars in the Sloan Digital Sky Survey (SDSS) Data Release 6 (DR6) is presented.
Abazajian+30 more
core +2 more sources
We report the discovery of COOL J0335−1927, a quasar at z = 3.27 lensed into three images with a maximum separation of 23.″3 by a galaxy cluster at z = 0.4178. To date, this is the highest redshift wide-separation lensed quasar known.
Kate Napier+20 more
doaj +1 more source
Preliminary Target Selection for the DESI Quasar (QSO) Sample [PDF]
The DESI survey will measure large-scale structure using quasars as direct tracers of dark matter in the redshift range 0.9 < z < 2.1 and using quasar Lyα forests at z > 2.1. We present two methods to select candidate quasars for DESI based on imaging in
C. Yéche+26 more
semanticscholar +1 more source
Two Close Separation Quasar-Quasar Pairs in the Large Bright Quasar Survey [PDF]
Accepted for publication in the Astronomical Journal, Paper, 4 Figures + 1 ...
Margaret E. Harding+5 more
openaire +3 more sources
Autosomal Dominant Leukodystrophy: A Disease of the Nuclear Lamina
The nuclear lamina is a fibrous meshwork of proteins found adjacent to the inner nuclear membrane that plays a critical role in the maintenance of nuclear architecture.
Quasar S. Padiath
doaj +1 more source
The Sloan Digital Sky Survey Quasar Catalog: Twelfth data release [PDF]
We present the Data Release 12 Quasar catalog (DR12Q) from the Baryon Oscillation Spectroscopic Survey (BOSS) of the Sloan Digital Sky Survey III. This catalog includes all SDSS-III/BOSS objects that were spectroscopically targeted as quasar candidates ...
I. Pâris+52 more
semanticscholar +1 more source
Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). V. Quasar Luminosity Function and Contribution to Cosmic Reionization at z = 6 [PDF]
We present new measurements of the quasar luminosity function (LF) at z ∼ 6 over an unprecedentedly wide range of the rest-frame ultraviolet luminosity M1450 from −30 to −22 mag.
Y. Matsuoka+46 more
semanticscholar +1 more source
In the quarter century since the first optical identification of a "radio star" (3C 48), astronomers have come to general agreement that the underlying quasar energy source is accretion onto a massive black hole. There is much less agreement on the detailed physics of the processes by which this energy is converted to the forms observed, but this has ...
Trimble, Virginia, Woltjer, Lodewijk
openaire +5 more sources
Quasars Probing Quasars. I. Optically Thick Absorbers near Luminous Quasars [PDF]
With close pairs of quasars at different redshifts, a background quasar sightline can be used to study a foreground quasar's environment in absorption. We search 149 moderate resolution background quasar spectra, from Gemini, Keck, the MMT, and the SDSS to survey Lyman Limit Systems (LLSs) and Damped Ly-alpha systems (DLAs) in the vicinity of 1.8 < ...
Scott Burles+13 more
openaire +4 more sources
Circum-Galactic Medium in the Halo of Quasars
The properties of circum-galactic gas in the halo of quasar host galaxies are investigated analyzing Mg II 2800 and C IV 1540 absorption-line systems along the line of sight close to quasars.
Riccardo Ottolina+6 more
doaj +1 more source