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We report the discovery of the first known probable case of a physical triple quasar (not a gravitational lens). A previously known double system, QQ 1429-008 at z = 2.076, is shown to contain a third, fainter QSO component at the same…

天体物理学 · 物理学 2009-11-13 S. G. Djorgovski , F. Courbin , G. Meylan , D. Sluse , D. J. Thompson , A. Mahabal , E. Glikman

We report a discovery of a quasar at z = 4.96 +- 0.03 within a few Mpc of the quasar SDSS 0338+0021 at z = 5.02 +- 0.02. The newly found quasar has the SDSS i and z magnitudes of ~ 21.2, and an estimated absolute magnitude M_B ~ -25.2. The…

天体物理学 · 物理学 2009-11-10 S. G. Djorgovski , D. Stern , A. Mahabal , R. Brunner

We report the discovery of a pair of z = 4.25 quasars with a separation of 33 arcseconds. The brighter of the two objects was identified as a high-redshift quasar candidate from Sloan Digital Sky Survey multicolor imaging data, and the…

We report the discovery of a quasar pair at z=5 separated by 21 arcsec. Both objects were identified as quasar candidates using simple color selection techniques applied to photometric catalogs from the CFHT Legacy Survey (CFHTLS). Spectra…

星系天体物理 · 物理学 2016-03-09 Ian McGreer , Sarah Eftekharzadeh , Adam Myers , Xiaohui Fan

Chandra snapshot observations of the three most distant quasars then known, at redshifts 5.82, 5.99, and 6.28, gave signficant detections even in the short, 6 -- 8 ks, observations. The X-ray to optical luminosity ratios indicate that…

天体物理学 · 物理学 2007-05-23 D. A. Schwartz , C. C. Cheung , J. F. C. Wardle

We report the discovery, spectroscopic confirmation, and mass modelling of the gravitationally lensed quasar system PS J0630-1201. The lens was discovered by matching a photometric quasar catalogue compiled from Pan-STARRS and WISE…

All galaxies once passed through a hyperluminous quasar phase powered by accretion onto a supermassive black hole. But because these episodes are brief, quasars are rare objects typically separated by cosmological distances. In a survey for…

星系天体物理 · 物理学 2015-05-15 Joseph F. Hennawi , J. Xavier Prochaska , Sebastiano Cantalupo , Fabrizio Arrigoni-Battaia

We have conducted an optical and infrared imaging in the neighbourhoods of 4 triplets of quasars. R, z', J and Ks images were obtained with MOSAIC II and ISPI at Cerro Tololo Interamerican Observatory. Accurate relative photometry and…

We present an investigation of the environment (\approx 600 kpc radius) of a pair of luminous z=4.25 quasars, SDSS J1439-0034 A,B, separated by 33''. An analysis of high-quality Subaru spectra of the quasars suggests that this configuration…

天体物理学 · 物理学 2009-11-10 Masataka Fukugita , Osamu Nakamura , Donald P. Schneider , Mamoru Doi , Nobunari Kashikawa

We have obtained follow-up observations of the quasar pair LBQS 0107-025A,B and new observations of the nearby quasar LBQS 0107-0232 with the Hubble Space Telescope Faint Object Spectrograph. Extended wavelength coverage of LBQS 0107-025A…

天体物理学 · 物理学 2014-10-13 P. A. Young , C. D. Impey , C. B. Foltz

We report the discovery of a unique gravitational lens system, SDSSJ2222+2745, producing five spectroscopically confirmed images of a z_s=2.82 quasar lensed by a foreground galaxy cluster at z_l=0.49. We also present photometric and…

In the third paper from the COOL-LAMPS Collaboration, we report the discovery of COOL J0542-2125, a gravitationally lensed quasar at $z=1.84$, observed as three images due to an intervening massive galaxy cluster at $z=0.61$. The lensed…

Binary quasars are extremely rare objects, used to investigate clustering on very small scales at different redshifts. The cases where the two quasar components are gravitationally bound, known as physical binary quasars, can also exhibit…

The strange morphology of the six-component gravitational lens PMN J0134-0931 has resisted explanation. We present the first successful quantitative models for the system, based on the idea that there are two lens galaxies and two…

天体物理学 · 物理学 2008-11-26 Charles R. Keeton , Joshua N. Winn

We report the discovery of a pair of quasars at $z=1.487$, with a separation of $8\farcs585\pm0\farcs002$. Subaru Telescope infrared imaging reveals the presence of an elliptical and a disk-like galaxy located almost symmetrically between…

宇宙学与河外天体物理 · 物理学 2015-06-05 Cristian E. Rusu , Masamune Oguri , Masanori Iye , Naohisa Inada , Issha Kayo , Min-Su Shin , Dominique Sluse , Michael A. Strauss

We report the discovery of a new quadruply imaged quasar surrounded by an optical Einstein ring candidate. Spectra of the different components of 1RXS J113155.4-123155 reveal a source at z=0.658. Up to now, this object is the closest known…

天体物理学 · 物理学 2009-11-10 D. Sluse , J. Surdej , J. -F. Claeskens , D. Hutsemekers , C. Jean , F. Courbin , T. Nakos , M. Billeres , S. V. Khmil

We present spectroscopic observations with Keck/LRIS of LBQS 0015+0239, a pair of quasars at z = 2.45 with a separation of $\Delta\theta = 2.2$ arcsec (projected linear distance of 17.8 $h_{70}^{-1}$ kpc, for $\Omega_m = 0.3$, $\Lambda =…

天体物理学 · 物理学 2014-10-13 C. D. Impey , C. E. Petry , C. B. Foltz , P. C. Hewett , F. H. Chaffee

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. In…

The quasar SDSS J153636.22+044127.0, exhibiting peculiar broad emission-line profiles with multiple components, was proposed as a candidate sub-parsec binary supermassive black hole system. More recently, imaging revealed two spatially…

宇宙学与河外天体物理 · 物理学 2015-05-13 Ryan Chornock , J. S. Bloom , S. B. Cenko , A. V. Filippenko , J. M. Silverman , M. D. Hicks , K. J. Lawrence , A. J. Mendez , M. Rafelski , A. M. Wolfe , ;

We report the discovery of a cluster of galaxies in the field of UM425, a pair of quasars separated by 6.5arcsec. Based on this finding, we revisit the long-standing question of whether this quasar pair is a binary quasar or a…

天体物理学 · 物理学 2009-11-11 Paul J. Green , Leopoldo Infante , Sebastian Lopez , Thomas L. Aldcroft , Josh N. Winn
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