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相关论文: The Central Component of Gravitational Lens Q0957+…

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We have produced deep radio maps of the double quasar 0957+561 from multiple-epoch VLA observations. To achieve high sensitivity to extended structure we have re-reduced the best available 1.6 GHz observations and have combined 5 GHz data…

天体物理学 · 物理学 2009-10-30 I. M. Avruch , A. S. Cohen , J. Lehar , S. R. Conner , D. B. Haarsma , B. F. Burke

The V=16.9 quasar FBQ 0951+2635 at redshift z=1.24 appears double on CCD exposures taken in subarcsecond seeing. The two objects are separated by 1.1" and differ in brightness by 0.9 mag. VLA observations show the radio source to be double…

天体物理学 · 物理学 2009-10-30 Paul L. Schechter , Michael D. Gregg , Robert H. Becker , David J. Helfand , Richard L. White

We present new spectroscopic and polarimetric observations of the first discovered gravitational lens Q0957+561 obtained with the 6m telescope of the Special Astrophysical Observatory (SAO, Russia). We explore spectropolarimetric parameters…

星系天体物理 · 物理学 2021-03-17 L. Č. Popović , V. L. Afanasiev , E. S. Shablovinskaya , V. I. Ardilanov , Dj. Savić

Q0957+561 was the first discovered gravitationally lensed quasar. The mirage shows two images of a radio-loud quasar at redshift z = 1.41. The time lag between these two images is well established around one year. We detected a very…

星系天体物理 · 物理学 2015-06-03 L. J. Goicoechea , V. N. Shalyapin , R. Gil-Merino , V. F. Braga

New HST WFPC2 observations of the lensed double QSO 0957+561 will allow improved constraints on the lens mass distribution and hence will improve the derived value of H$_0$. We first present improved optical positions and photometry for the…

天体物理学 · 物理学 2009-10-30 Gary Bernstein , Philippe Fischer , J. Anthony Tyson , George Rhee

We report the discovery of a new gravitationally lensed radio source. Radio maps of MG0751+2716 show four lensed images, which, at higher resolution, are resolved into long arcs of emission. A group of galaxies is present in optical images,…

We report the discovery of a gravitationally lensed quasar resulting from our survey for lenses in the southern sky. Radio images of PMN J1632-0033 with the VLA and ATCA exhibit two compact, flat-spectrum components with separation 1.47"…

A single-screen model of the gravitational lens system 2016+112 is proposed, that explains recent Hubble Space Telescope} (HST) infrared (NICMOS-F160W) observations and new high-resolution European VLBI Network (EVN) 5-GHz radio…

天体物理学 · 物理学 2009-11-06 L. V. E. Koopmans , M. A. Garrett , R. D. Blandford , C. R. Lawrence , A. R. Patnaik , R. W. Porcas

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 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…

We present e-MERLIN and EVN observations which reveal unambiguous jet activity within radio quiet quasar HS~0810+2554. With an intrinsic flux density of 880~nJy, this is the faintest radio source ever imaged. The findings present new…

星系天体物理 · 物理学 2019-03-06 P. Hartley , N. Jackson , D. Sluse , H. R. Stacey , H. Vives-Arias

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

We present our ground-based optical imaging, spectral analysis, and high resolution radio mapping of the gravitational lens candidate FBQ 1633+3134. This z=1.52, B=17.7 quasar appears double on CCD images with an image separation of 0.66…

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

The radio-loud quasar PMN J0134-0931 was discovered to have an unusual morphology during our search for gravitational lenses. In VLA and MERLIN images, there are 5 compact components with maximum separation 681 millarcseconds. All of these…

We present radio, optical, near-infrared and spectroscopic observations of the source B0827+525. We consider this source as the best candidate from the Cosmic Lens All-Sky Survey (CLASS) for a `dark lens' system or binary radio-loud quasar.…

A doubly-peaked quasar microlensing event in the lensed Twin Quasar Q0957+561 A,B (Colley and Schild 2003) is analysed within several lensing models. In the most realistic model a lens resolves in image B the ellipse shaped, bright inner…

星系天体物理 · 物理学 2021-07-28 Theodorus M. Nieuwenhuizen

We present new long-slit William Herschel Telescope spectroscopic observations of the lens galaxy G1 associated with the double-imaged QSO 0957+561A,B. The obtained central stellar velocity dispersion, sigma_l = 310 +/- 20 km/s, is in…

天体物理学 · 物理学 2009-10-31 E. Mediavilla , M. Serra-Ricart , A. Oscoz , L. J. Goicoechea , J. Buitrago

We present milliarcsecond (mas) angular resolution observations of the gravitationally lensed radio source MG J0751+2716 (at z=3.2) obtained with global Very Long Baseline Interferometry (VLBI) at 1.65 GHz. The background object is highly…

星系天体物理 · 物理学 2018-07-17 C. Spingola , J. P. McKean , M. W. Auger , C. D. Fassnacht , L. V. E. Koopmans , D. J. Lagattuta , S. Vegetti

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
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