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We present the first unambiguous case of external variability of a radio gravitational lens, CLASS B1600+434. The VLA 8.5-GHz difference light curve of the lensed images, taking the proper time-delay into account, shows the presence of…

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

We present polarisation observations of the gravitational lens system B1422+231 made at 8.4 GHz using the VLBA and the 100m telescope at Effelsberg. All four images of the quasar show structure on the milliarcsec scale. The three bright…

天体物理学 · 物理学 2009-10-31 A. R. Patnaik , A. J. Kemball , R. W. Porcas , M. A. Garrett

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

Strongly correlated non-intrinsic variability between 5 and 8.5 GHz has been observed in one of the lensed images of the gravitational lens B1600+434. These non-intrinsic (i.e. `external') variations are interpreted as `radio-microlensing'…

We report the discovery of a new double image gravitational lens system B1030+074 which was found during the Jodrell Bank - VLA Astrometric Survey (JVAS). We have collected extensive radio data on the system using the VLA, MERLIN, the EVN…

First, we review the current status of the detection of strong `external' variability in the CLASS gravitational B1600+434, focusing on the 1998 VLA 8.5-GHz and 1998/9 WSRT multi-frequency observations. We show that this data can best be…

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

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

We present new observations of the gravitational lens (GL) system B1600+434, strongly suggesting that the lens is an edge-on spiral galaxy. These observations are used to constrain the mass model of the system, in particular the oblateness…

天体物理学 · 物理学 2009-10-30 L. V. E. Koopmans , A. G. de Bruyn , N. Jackson

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 the first unambiguous case of external variability of an extra-galactic radio source, the CLASS gravitational lens B1600+434, consisting of two images lensed by an edge-on disk galaxy. The VLA 8.5-GHz difference light curve of…

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

We report the discovery of a new gravitational lens system from the CLASS survey. Radio observations with the VLA, the WSRT and MERLIN show that the radio source B0850+054 is comprised of two compact components with identical spectra, a…

We report the discovery of a new two-image gravitational lens system from the Cosmic Lens All-Sky Survey, CLASS B2319+051. Radio imaging with the Very Large Array (VLA) and Multi-Element Radio-Linked Interferometer Network (MERLIN) shows…

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

Gravitational lensing is a powerful tool for quantifying the mass content and distribution in distant galaxies. By using milliarcsecond angular resolution observations of radio-loud gravitationally lensed sources it is also possible to…

星系天体物理 · 物理学 2019-02-20 C. Spingola , J. P. McKean , A. Deller , J. Moldon

We discuss the gravitational lensing of gravitational wave signals from coalescing binaries. We delineate the regime where wave effects are significant from the regime where geometric limit can be used. Further, we focus on the effect of…

宇宙学与河外天体物理 · 物理学 2019-12-18 Ashish Kumar Meena , J S Bagla

We present new observations of the gravitational lens system CLASS B0128+437. HST observations detect a very faint, extended object in I-band with no emission from the lensed images visible; no detection at all is made in V-band. The lens…

天体物理学 · 物理学 2007-05-23 A. D. Biggs , I. W. A. Browne , N. J. Jackson , T. York , M. A. Norbury , J. P. McKean , P. M. Phillips

We present Global VLBI and HSA images of the gravitational lens B2016+112 at 18, 6 and 3.6 cm. Previous VLBI observations showed that images A and B (which are clearly lensed images of a single background source) and the elongated region C…

天体物理学 · 物理学 2007-05-23 A. More , R. W. Porcas

The four-image gravitational lens system MG0414+0534 was observed with the VLA at 1.4, 5, 8, 15, and 22 GHz. The 15 and 22 GHz images reveal structure in the components which is consistent with that seen at other wavelengths. There was no…

天体物理学 · 物理学 2009-10-28 C. A. Katz , C. B. Moore , J. N. Hewitt

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…

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
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