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相关论文: J0316+4328: a Probable "Asymmetric Double" Lens

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We present results from a systematic search for strong gravitational lenses in the GOODS ACS data. The search technique involves creating a sample of likely lensing galaxies, which we define as massive early-type galaxies in a redshift…

天体物理学 · 物理学 2009-11-10 C. D. Fassnacht , L. A. Moustakas , S. Casertano , H. C. Ferguson , R. A. Lucas , Y. Park

We present long-baseline ALMA observations of the strong gravitational lens H-ATLAS J090740.0-004200 (SDP.9), which consists of an elliptical galaxy at $z_{\mathrm{L}}=0.6129$ lensing a background submillimeter galaxy into two extended…

星系天体物理 · 物理学 2017-07-26 Kenneth C. Wong , Tsuyoshi Ishida , Yoichi Tamura , Sherry H. Suyu , Masamune Oguri , Satoki Matsushita

We address the issue of anomalous image flux ratios seen in the double-image gravitational lens JVAS B0218+357. From the multi-frequency observations presented in a recent study (Mittal et al. 2006) and several previous observations made by…

天体物理学 · 物理学 2009-11-11 Rupal Mittal , Richard Porcas , Olaf Wucknitz

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

Gravitational lensing is an important tool for probing the mass distribution of galaxies. In this letter we report the discovery of a new quadruple lens HST 1411+5211 found in archived WFPC2 images of the galaxy cluster CL140933+5226. If…

天体物理学 · 物理学 2009-10-30 Philippe Fischer , David Schade , Felipe Barientos

Substructure in distant gravitational lens galaxies can be detected because it alters the brightnesses and shapes of the lensed images. The optical and radio flux ratios in the four-image lens B1422+231 imply that there is a \sim 10^4-10^7…

天体物理学 · 物理学 2007-05-23 Charles R. Keeton

We report the discovery of a new gravitationally lensed quasar, SDSS J131339.98+515128.3, at a redshift of 1.875 with an image separation of 1.24". The lensing galaxy is clearly detected in visible-light follow-up observations. We also…

天体物理学 · 物理学 2009-06-23 E. O. Ofek , M. Oguri , N. Jackson , N. Inada , I. Kayo

We examine the possibility of observing gravitational lensing in the weak deflection regime by the supermassive black hole in the center of the galaxy M31. This black hole is significantly more massive than the black hole in the center of…

天体物理学 · 物理学 2009-06-23 V. Bozza , S. Calchi Novati , L. Mancini

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 the discovery of four gravitationally lensed quasars selected from the spectroscopic quasar catalog of the Sloan Digital Sky Survey. We describe imaging and spectroscopic follow-up observations that support the lensing…

We present the first result of a survey for strong galaxy-galaxy lenses in Sloan Digital Sky Survey (SDSS) images. SDSS J082728.70+223256.4 was selected as a lensing candidate using selection criteria based on the color and positions of…

SDSS J0924+0219 is the most glaring example of a gravitational lens with anomalous flux ratios: optical broad-band photometry shows image D to be a factor of 12 fainter than expected for smooth lens potentials. We report spectroscopy…

天体物理学 · 物理学 2009-11-13 Charles R. Keeton , Scott Burles , Paul L. Schechter , Joachim Wambsganss

We report on the results of a spectroscopic survey of the environments of the gravitational lens systems CLASS B1600+434 (z_l = 0.41, z_s = 1.59) and CLASS B2319+051 (z_l = 0.62). The B1600+434 system has a time delay measured for it, and…

天体物理学 · 物理学 2008-11-26 M. W. Auger , C. D. Fassnacht , A. L. Abrahamse , L. M. Lubin , G. K. Squires

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

A complete manual search has been carried out of the list of 285423 objects, nearly all of them galaxies, identified in the COSMOS field that are brighter than I=25. Two certain and one highly probable new gravitational lenses are found, in…

天体物理学 · 物理学 2009-11-13 Neal Jackson

Our aim was to identify gravitational lens candidates among some 5500 optical counterparts of the X-ray point-like sources in the medium-deep ~11 sq. deg. XMM-LSS survey. We have visually inspected the optical counterparts of each QSOs/AGN…

宇宙学与河外天体物理 · 物理学 2015-06-16 A. Elyiv , O. Melnyk , F. Finet , A. Pospieszalska-Surdej , L. Chiappetti , M. Pierre , T. Sadibekova , J. Surdej

The third phase of the Cosmic Lens All-Sky Survey (CLASS) has recently been completed, bringing the total number of sources imaged to over 15000 in the CLASS and JVAS combined survey. In the VLA observations carried out in March and April…

We present the strategy and status of a gravitational lens search for multiple imaging with angular separations between 6'' and 15'' with the combined JVAS and CLASS data set of ~15,000 flat-spectrum radio sources. Currently all but one…

天体物理学 · 物理学 2007-05-23 P. M. Phillips , I. W. A. Browne , P. N. Wilkinson , N. J. Jackson

We observed the quadruple gravitationally lensed image of MGJ0414+0534 on 23 November 1997 with a global VLBI array at 8.4 GHz. We report wide-field imaging results of its four components at submilliarcsecond resolution, displaying complex…

天体物理学 · 物理学 2007-05-23 E. Ros , J. C. Guirado , J. M. Marcaide , M. A. Perez-Torres , E. E. Falco , J. A. Munoz , A. Alberdi , L. Lara

We present Low-Frequency Array (LOFAR) telescope observations of the radio-loud gravitational lens systems MG 0751+2716 and CLASS B1600+434. These observations produce images at 300 milliarcseconds (mas) resolution at 150 MHz. In the case…