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相关论文: Detection of the lensing galaxy in HE 2149-2745

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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 report the discovery of the new gravitational lens system HE~0230$-$2130, a QSO at redshift $z=2.162$ consisting of at least five distinct components. Three of these are clearly lensed images of the QSO, one is most likely the lensing…

天体物理学 · 物理学 2007-05-23 L. Wisotzki , N. Christlieb , M. C. Liu , J. Maza , N. D. Morgan , P. L. Schechter

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 report the discovery of a new gravitationally lensed QSO, at a redshift z = 1.689, with four QSO components in a cross-shaped arrangement around a bright galaxy. The maximum separation between images is 2.6 arcsec, enabling a reliable…

天体物理学 · 物理学 2009-11-07 Lutz Wisotzki , Paul L. Schechter , Hale V. Bradt , Janine Heinmueller , Dieter Reimers

We report on deep IR imaging of the double quasar HE 1104-1805. A new image deconvolution technique has been applied to the data in order to optimally combine the numerous frames obtained. The resulting J and K' images allow us to detect…

天体物理学 · 物理学 2009-09-25 F. Courbin , C. Lidman , P. Magain

Aims. Falomo et al. (2005) discovered a disk-like galaxy at ~ 1.2 arcsec from the QSO Q0045-3337 by means of ESO VLT adaptive optics. They estimated a galaxy Einstein radius (for a point mass) of comparable size, thus pointing up the…

天体物理学 · 物理学 2010-01-15 M. Chieregato , M. Miranda , P. Jetzer

We present the first spatially resolved spectroscopic observations of the recently discovered quadruple QSO and gravitational lens HE0435-1223. Using the Potsdam Multi-Aperture Spectrophotometer (PMAS), we show that all four QSO components…

天体物理学 · 物理学 2009-11-10 L. Wisotzki , T. Becker , L. Christensen , A. Helms , K. Jahnke , A. Kelz , M. M. Roth , S. F. Sanchez

H band observations with a spatial resolution of 0.15" carried out with the Canada-France-Hawaii Telescope adaptive optics system show a galaxy between the components of the double BAL quasar SBS 1520+530, thereby confirming this system as…

天体物理学 · 物理学 2009-10-30 David Crampton , P. L. Schechter , J. -L. Beuzit

The quasar Q1208+1011 (z_{em}=3.8) is the second highest redshift double quasar ever detected. Several indications point toward it being a gravitational lensed system, although a definitive proof is still lacking. We present new evidence of…

天体物理学 · 物理学 2009-10-30 E. Giallongo , A. Fontana , S. Cristiani , S. D'Odorico

We present the first lensing total mass estimate of a galaxy, at redshift 2.207, that acts as a gravitational deflector and damped Lyman-alpha absorber on the background QSO SDSS J1135-0010, at redshift 2.888. The remarkably small projected…

宇宙学与河外天体物理 · 物理学 2015-06-18 C. Grillo , J. P. U. Fynbo

High angular resolution images of the complex gravitational lens system RXS J1131-1231 (a quadruply imaged AGN with a bright Einstein ring) obtained with the Advanced Camera for Surveys and NICMOS instruments onboard the Hubble Space…

天体物理学 · 物理学 2009-11-11 J. -F. Claeskens , D. Sluse , P. Riaud , J. Surdej

We have discovered strong gravitational lensing by the galaxy ESO325-G004, in images obtained with the Advanced Camera for Surveys on the Hubble Space Telescope. The lens galaxy is a boxy group-dominant elliptical at z=0.0345, making this…

天体物理学 · 物理学 2009-11-11 Russell J. Smith , John P. Blakeslee , John R. Lucey , John Tonry

We present spectra of QSOs 1343+266 A B, covering Ly-beta to C~IV emission at 2\AA~resolution, and find further evidence that this system is not gravitationally lensed. We see, however, a large number of Ly-alpha and some C~IV absorption…

天体物理学 · 物理学 2009-10-22 Arlin P. S. Crotts , Jill Bechtold , Yihu Fang , Robert C. Duncan

The quasar HE 0047-1756, at z=1.67, is found to be split into two images 1.44" apart by an intervening galaxy acting as a gravitational lens. The flux ratio for the two components is roughly 3.5:1, depending slightly upon wavelength. The…

We report the discovery of a new two-image gravitationally lensed quasar, SDSS J024634.11-082536.2 (SDSS J0246-0825). This object was selected as a lensed quasar candidate from the Sloan Digital Sky Survey (SDSS) by the same algorithm that…

The gravitational lens system CLASS B2108+213 has two lensed images separated by 4.56 arcsec. Such a wide image separation suggests that the lens is either a massive galaxy, or is composed of a group of galaxies. To investigate the…

天体物理学 · 物理学 2009-11-13 A. More , J. P. McKean , T. W. B. Muxlow , R. W. Porcas , C. D. Fassnacht , L. V. E. Koopmans

We have measured a velocity dispersion for the foreground galaxy in this gravitationally lensed system. Our dispersion confirms the prediction from lens models, provided that the source is distant enough ($z_{_S}>0.2$). Current…

天体物理学 · 物理学 2009-10-28 J. Lehar , A. J. Cooke , C. R. Lawrence , A. D. Silber , G. I. Langston

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

The quasar SDSS J133401.39+331534.3 at z = 2.426 is found to be a two-image gravitationally lensed quasar with the image separation of 0.833. The object is first identified as a lensed quasar candidate in the Sloan Digital Sky Survey Quasar…

We present high-resolution CCD images (FWHM=0.6"-0.7") of the compact gravitational lens system B0218+35.7 obtained at the Nordic Optical Telescope. Using aperture and PSF photometry we detect the two closely separated (335 mas) components…

天体物理学 · 物理学 2016-06-08 F. Grundahl , J. Hjorth
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