English
Related papers

Related papers: Cosmic alignment towards the radio Einstein ring P…

200 papers

We report the serendipitous discovery of an "Einstein Ring" in the optical band from the Sloan Digital Sky Survey (SDSS) data and associated four images of a background source. The lens galaxy appears to be a nearby dwarf spheroid at a…

Astrophysics · Physics 2011-02-11 Kajal K Ghosh , D. Narasimha

Time variability of astronomical sources provides crude information on their typical size and on the implied physical mechanisms. PKS1830-211 is a remarkable radio-bright lensed quasar with a foreground molecular absorber at z=0.89.…

Astrophysics of Galaxies · Physics 2024-09-02 S. Muller , I. Marti-Vidal , F. Combes , M. Gerin , A. Beelen , C. Horellou , M. Guelin , S. Aalto , J. H. Black , E. van Kampen

Westerbork Radio Synthesis Telescope observations of the redshifted 21cm line absorber against the z_em = 0.871 double lobed quasar 3C196 show that the intervening absorber is an L approximately equal L* spiral galaxy (3C196-G1) and that…

Astrophysics · Physics 2009-11-06 F. H. Briggs , A. G. de Bruyn , R. C. Vermeulen

(Abridged) A new technique for the spatial deconvolution of spectra is applied to near-IR (0.95 - 2.50 micron) NTT/SOFI spectra of the lensed, radio-quiet quasar HE 1104-1805. The continuum of the lensing galaxy is revealed between 1.5 and…

Astrophysics · Physics 2007-05-23 F. Courbin , C. Lidman , G. Meylan , J. -P. Kneib , P. Magain

We present a high-resolution spectrum of the high redshift, lensed quasar Q1208+1101, obtained with the echellette spectrograph on the Multiple Mirror Telescope. We examine the new and published spectra and provide an updated list of…

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…

Astrophysics · Physics 2009-06-23 E. O. Ofek , M. Oguri , N. Jackson , N. Inada , I. Kayo

We present a source and lens reconstruction for the optical Einstein ring gravitational lens system RXS J1131-1231. We resolve detail in the source, which is the host galaxy of a $z=0.658$ quasar, down to a resolution of 0.045 arc seconds…

Astrophysics · Physics 2009-11-13 Brendon J. Brewer , Geraint F. Lewis

Gravitational microlensing has proven to be a powerful probe of both the structure at the heart of quasars and the mass function of compact objects in foreground lenses. This paper examines the potential of gravitational microlensing in…

Astrophysics · Physics 2009-11-07 Geraint F. Lewis , Rodrigo A. Ibata

We report the discovery of a z=2.65 low-ionization iron broad absorption line quasar, FIRST J100424.9+122922, which is gravitationally-lensed by a galaxy at z~0.95. The object was discovered as part of a program to find very red quasars by…

Astrophysics · Physics 2009-11-07 M. Lacy , M. Gregg , R. H. Becker , R. L. White , E. Glikman , D. Helfand , J. 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…

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…

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

We discuss BIMA (Berkeley Illinois Maryland Association) data and present new high quality optical and near-IR Keck images of the bright radio ring PKS 1830-211. Applying a powerful new deconvolution algorithm we have been able to identify…

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…

Hubble Space Telescope observations of the gravitational lens PG 1115+080 in the infrared show the known z =0.310 lens galaxy and reveal the z = 1.722 quasar host galaxy. The main lens galaxy G is a nearly circular (ellipticity < 0.07)…

Astrophysics · Physics 2009-10-30 C. Impey , E. Falco , C. Kochanek , J. Lehar , B. McLeod , H. -W. Rix , C. Peng , C. Keeton

Absorption spectroscopy of gravitationally lensed quasars (GLQs) enables study of spatial variations in the interstellar and/or circumgalactic medium of foreground galaxies. We report observations of 4 GLQs, each with two images separated…

Some recent work on radio source fields at z~0.7 and z~4 is discussed. At z~0.7 we find that radio-loud quasars are typically found in moderately rich environments independent of radio luminosity, consistent with previous results at z~0.5.…

Astrophysics · Physics 2007-05-23 M. Lacy

Based on measurements with the Effelsberg 100-m telescope, a multi-line study of molecular species is presented toward the south-western source of the gravitational lens system PKS 1830-211, which is by far the best known target to study…

Astrophysics of Galaxies · Physics 2015-02-04 A. Schulz , C. Henkel , K. M. Menten , S. Muller , D. Muders , J. Bagdonaite , W. Ubachs

We present optical spectroscopic and milli-arcsecond scale radio continuum observations of the quasar M1540-1453 ($z_{em}$ = 2.104$\pm$0.002) that shows associated HI 21-cm absorption at $z_{abs}$ = 2.1139. At sub-kpc scales, the powerful…

Astrophysics of Galaxies · Physics 2022-03-30 N. Gupta , R. Srianand , E. Momjian , G. Shukla , F. Combes , J. -K. Krogager , P. Noterdaeme , P. Petitjean

We present the discovery and preliminary characterization of a gravitationally lensed quasar with a source redshift $z_{s}=2.74$ and image separation of $2.9"$ lensed by a foreground $z_{l}=0.40$ elliptical galaxy. Since the images of…

We present the results of the first long-term (2.2 years) spectroscopic monitoring of a gravitationally lensed quasar, namely the Einstein Cross Q2237+0305. We spatially deconvolve deep VLT/FORS1 spectra to accurately separate the spectrum…

Astrophysics · Physics 2009-04-14 A. Eigenbrod , F. Courbin , D. Sluse , G. Meylan , E. Agol