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相关论文: CLASS B0739+366: A new two-image gravitational len…

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The gravitationally lensed quasar B1600+434 (z=1.61, mV=21.6) has been observed at the 2.56m Nordic Optical Telescope (NOT). In this Letter we report the discovery of an edge-on late-type galaxy located between the two lensed components…

天体物理学 · 物理学 2011-05-23 A. O. Jaunsen , J. Hjorth

We present a multi-wavelength study of the gravitational lens COSMOS J095930+023427 (z=0.89), together with the associated galaxy group located at $z\sim0.7$ along the line of sight and the lensed background galaxy. The source redshift is…

宇宙学与河外天体物理 · 物理学 2015-06-12 Shuo Cao , Giovanni Covone , Maurizio Paolillo , Zong-Hong Zhu

We report the discovery of four groups of galaxies along the line of sight to the B1608+656 gravitational lens system. One group is at the redshift of the primary lensing galaxy (z = 0.631) and appears to have a low mass, with eight…

天体物理学 · 物理学 2009-11-13 C. D. Fassnacht , R. R. Gal , L. M. Lubin , J. P. McKean , G. K. Squires , A. C. S. Readhead

We have reanalysed the 1996/1997 VLA monitoring data of the gravitational lens system JVAS B0218+357 to produce improved total flux density and polarization variability curves at 15, 8.4 and 5 GHz. This has been done using improved…

宇宙学与河外天体物理 · 物理学 2018-03-21 A. D. Biggs , I. W. A. Browne

Strong gravitational lens systems with measured time delays between the multiple images provide a method for measuring the "time-delay distance" to the lens, and thus the Hubble constant. We present a Bayesian analysis of the strong…

宇宙学与河外天体物理 · 物理学 2010-12-08 S. H. Suyu , P. J. Marshall , M. W. Auger , S. Hilbert , R. D. Blandford , L. V. E. Koopmans , C. D. Fassnacht , T. Treu

We report the discovery of a new two-image gravitational lens candidate. The system RX J0921+4529 contains two z_s=1.66 quasars separated by 6."93 with an H band magnitude difference of $\Delta m=1.39$. The HST NIC2 H band images reveal an…

We present new VLA 22-GHz and e-MERLIN 5-GHz observations of CLASS B1030+074, a two-image strong gravitational lens system whose background source is a compact flat-spectrum radio quasar. In such systems we expect a third image of the…

We present Very Large Array (VLA) 8.5-GHz light curves of the two lens images of the Cosmic Lens All Sky Survey (CLASS) gravitational lens B1600+434. We find a nearly linear decrease of 18-19% in the flux densities of both lens images over…

天体物理学 · 物理学 2007-05-23 L. V. E. Koopmans , A. G. de Bruyn , E. Xanthopoulos , C. D. Fassnacht

We present observations of a new double-image gravitational lens system, ULAS J082016.1+081216, of image separation 2.3" and high (~6) flux ratio. The system is selected from the Sloan Digital Sky Survey spectroscopic quasar list using new…

宇宙学与河外天体物理 · 物理学 2010-11-02 Neal Jackson , Eran O. Ofek , Masamune Oguri

The complex ten-component gravitational lens system B1933+503 has been monitored with the VLA during the period February to June 1998 with a view to measuring the time delay between the four compact components and hence to determine the…

天体物理学 · 物理学 2009-10-31 A. D. Biggs , E. Xanthopoulos , I. W. A. Browne , L. V. E. Koopmans , C. D. Fassnacht

We report the discovery of a new double-image quasar that was found during a search for gravitational lenses in the southern sky. Radio source PMN J1838-3427 is composed of two flat-spectrum components with separation 1", flux density ratio…

LISA might detect gravitational waves from mergers of massive black hole binaries strongly lensed by intervening galaxies (Sereno et al. 2010). The detection of multiple gravitational lensing events would provide a new tool for cosmography.…

宇宙学与河外天体物理 · 物理学 2015-05-27 M. Sereno , Ph. Jetzer , A. Sesana , M. Volonteri

We report the discovery of two new gravitationally lensed quasars, WFI J2026-4536 and WFI J2033-4723, at respective source redshifts of z=2.23 and z=1.66. Both systems are quadruply imaged and have similar PG1115-like image configurations.…

In this paper we present new observations of the gravitational lens system JVAS B0218+357 made with a global VLBI network at a frequency of 8.4 GHz. Our maps have an rms noise of 30 microJy/beam and with these we have been able to image…

天体物理学 · 物理学 2007-05-23 A. D. Biggs , O. Wucknitz , R. W. Porcas , I. W. A. Browne , N. J. Jackson , S. Mao , P. N. Wilkinson

We present an analysis of archival multi-frequency Very Large Array monitoring data of the two-image gravitational lens system CLASS B1600+434, including the polarization properties at 8.5 GHz. From simulating radio light curves…

星系天体物理 · 物理学 2021-07-07 A. D. Biggs

We present adaptive optics imaging of the CLASS gravitational lens system B1359+154 obtained with the Canada-France-Hawaii Telescope (CFHT) in the infrared K band. The observations show at least three brightness peaks within the ring of…

天体物理学 · 物理学 2009-10-31 D. Rusin , P. B. Hall , R. C. Nichol , D. R. Marlow , A. M. S. Richards , S. T. Myers

We present a detailed mm-wave and optical study of the gravitational lens system B1933+503, discovered by Sykes et al.(1998) in the radio. This object is probably the most complex lens system known, with 10 lensed components within a radius…

天体物理学 · 物理学 2007-05-23 Scott C. Chapman , Douglas Scott , Geraint F. Lewis , Colin Borys , Gregory G. Fahlman

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 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

We present deep optical observations of the gravitational lens system CLASS B0218+357, from which we derive an estimate of the Hubble constant. Extensive radio observations have reduced the degeneracies between Hubble's constant and the…

天体物理学 · 物理学 2009-11-10 T. York , N. Jackson , I. W. A. Browne , O. Wucknitz , J. E. Skelton