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相关论文: Chandra Observations of the QSO Pair Q2345+007: Bi…

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We have obtained a 110 ksec Chandra ACIS-S exposure of UM425, a pair of QSOs at z=1.47 separated by 6.5 arcsec, which show remarkably similar emission and broad absorption line (BAL) profiles in the optical/UV. Our 5000 count X-ray spectrum…

天体物理学 · 物理学 2009-11-07 T. L. Aldcroft , P. J. Green

Luminous objects associated with the 7.06\arcsec\ separation double quasar Q2345+007 have, until now, escaped detection. In this letter we present the results of the deepest known imaging of the region surrounding the quasar. The total…

天体物理学 · 物理学 2009-10-22 Philippe Fischer , J. Anthony Tyson , Gary M. Bernstein , Puragra Guhathakurta

Deep HST/NICMOS H (F160W) band observations of the z=1.96 quasar pair Q 1634+267A,B reveal no signs of a lens galaxy to a 1 sigma threshold of approximately 22.5 mag. The minimum luminosity for a normal lens galaxy would be a 6L_* galaxy at…

天体物理学 · 物理学 2009-10-31 C. Y. Peng , C. D. Impey , E. E. Falco , C. S. Kochanek , J. Lehar , B. A. McLeod , H. -W. Rix , C. R. Keeton , J. A. Munoz

The double QSO2345+007 comprises two optical components separated by 7.1\ arcseconds and is the most prominent `dark matter' gravitational lens candidate. Despite being known for more than a decade, optical spectroscopy and imaging have…

天体物理学 · 物理学 2016-06-08 Alok R. Patnaik , Peter Schneider , Ramesh Narayan

We report the discovery of a new gravitational lens candidate Q2138-431AB, comprising two quasar images at a redshift of 1.641 separated by 4.5 arcsecs. The spectra of the two images are very similar, and the redshifts agree to better than…

天体物理学 · 物理学 2016-08-15 M. R. S. Hawkins , D. Clements , J. W. Fried , A. F. Heavens , P. Véron , E. M. Minty , P. van der Werf

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

An observation of the gravitationally lensed system 2016+112 with the Chandra X-ray Observatory has resolved a mystery regarding the proposed presence of a dark matter object in the lens plane of this system. The Chandra ACIS observation…

天体物理学 · 物理学 2009-11-06 G. Chartas , M. Bautz , G. Garmire , C. Jones , D. P. Schneider

(abridged) Steidel & Sargent (1991a) found that the spectra of the components of the close quasar pairs Q1634+267A,B and Q2345+007A,B were in each case remarkably similar but that individual broad emission lines due to Ly_alpha, Si IV, C…

天体物理学 · 物理学 2009-10-30 Todd A. Small , Wallace L. W. Sargent , Charles C. Steidel

We present results from Chandra observations of the cluster lens SDSS J1029+2623 at z_l=0.58, which is a gravitationally lensed quasar with the largest known image separation. We clearly detect X-ray emission both from the lensing cluster…

Very deep ESO/VLT FORS1 and ISAAC images, as well as HST NICMOS2 data are used to infer the nature of the quasar pair LBQS 1429-0053 A and B, either a binary quasar or a doubly-imaged lensed quasar. Direct search of a putative lensing…

天体物理学 · 物理学 2009-11-07 C. Faure , D. Alloin , S. Gras , F. Courbin , J. -P. Kneib , P. Hudelot

Quasar pairs are either physically distinct binary quasars or the result of gravitational lensing. The majority of known pairs are in fact lenses, with a few confirmed as binaries, leaving a population of objects that have not yet been…

天体物理学 · 物理学 2009-10-31 Daniel J. Mortlock , Rachel L. Webster , Paul J. Francis

We present the first results from a new survey for high-redshift $(z\gtrsim5)$ gravitationally lensed quasars and close quasar pairs. We carry out candidate selection based on the colors and shapes of objects in public imaging surveys, then…

星系天体物理 · 物理学 2023-04-12 Minghao Yue , Xiaohui Fan , Jinyi Yang , Feige Wang

We use simple comparisons of the optical and radio properties of the wide separation (3'' to 10'') quasar pairs to demonstrate that they are binary quasars rather than gravitational lenses. The most likely model is that all the pairs are…

天体物理学 · 物理学 2007-05-23 C. S. Kochanek , E. E. Falco , J. A. Munoz

We present results from Chandra observations of SDSS J1004+4112, a strongly lensed quasar system with a maximum image separation of 15". All four bright images of the quasar, as well as resolved X-ray emission originating from the lensing…

This paper reviews the question of whether the wide separation double quasar Q2138-431 is a gravitational lens. From early work, the two quasar images are known to have almost identical spectra and redshifts, but no lensing galaxy has so…

星系天体物理 · 物理学 2021-04-16 M. R. S. Hawkins

We present Chandra X-ray imaging and spectroscopy for 14 quasars in spatially resolved pairs, part of a complete sample of binary quasars with small transverse separations drawn from Sloan Digital Sky Survey (DR6) photometry. We find no…

We present deep Chandra observations of PSO J231.6576$-$20.8335, a quasar at redshift z=6.59 with a nearby (${\sim}8$ proper kpc) companion galaxy. ALMA observed both the quasar and companion to be bright in [C II], and the system has…

This paper describes new results on the identification of the complex gravita- tional lens responsible for the double quasar Q2345+007. A gravitational shear field was detected recently about 45'' away from the QSO, centered on an excess of…

天体物理学 · 物理学 2007-05-23 R. Pello , J. M. Miralles , J. -F. Le Borgne , J. -P. Picat , G. Soucail , G. Bruzual

More than $200$ quasars have been detected so far at $z > 6$, with only one showing clear signs of strong gravitational lensing. Some studies call for a missing population of lensed high-$z$ quasars, but their existence is still in doubt. A…

星系天体物理 · 物理学 2022-07-21 Fabio Pacucci , Adi Foord , Lucia Gordon , Abraham Loeb

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…

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