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Related papers: Mass and dust in the disk of a spiral lens galaxy

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We report the serendipitous discovery of a quadruply-lensed source behind the z=0.095 edge-on disk galaxy 2MASXJ13170000-1405187, based on public imaging survey data from Pan-STARRS PS1 and the VISTA Hemisphere Survey. Follow-up imaging…

Astrophysics of Galaxies · Physics 2018-06-20 John R. Lucey , Russell J. Smith , Paul L. Schechter , Amanda S. Bosh , Stephen E. Levine

Gravitational lensing of a quasar by a spiral galaxy should often be accompanied by damped Lyman-alpha absorption and dust extinction due to the intervening gaseous disk. In nearly edge-on configurations, the surface mass density of the gas…

Astrophysics · Physics 2009-10-30 Matthias Bartelmann , Abraham Loeb

We present new Hubble Space Telescope images of the gravitational lens PKS 1830-211, which allow us to characterize the lens galaxy and update the determination of the Hubble constant from this system. The I-band image shows that the lens…

Aims. Falomo et al. (2005) discovered a disk-like galaxy at ~ 1.2 arcsec from the QSO Q0045-3337 by means of ESO VLT adaptive optics. They estimated a galaxy Einstein radius (for a point mass) of comparable size, thus pointing up the…

Astrophysics · Physics 2010-01-15 M. Chieregato , M. Miranda , P. Jetzer

We present the CXOCY J220132.8-320144 system, which is composed of an edge-on spiral galaxy at z=0.32 lensing a z=3.9 background quasar. Two images of the quasar are seen. The geometry of the system is favorable to separate the relative…

Astrophysics · Physics 2009-11-11 F. J. Castander , E. Treister , J. Maza , E. Gawiser

We report the discovery of a new double-image gravitational lens resulting from our search for lenses in the southern sky. Radio source PMN J2004-1349 is composed of two compact components separated by 1.13 arcseconds in VLA, MERLIN and…

The CXOCY J220132.8-320144 system consists of an edge-on spiral galaxy lensing a background quasar into two bright images. Previous efforts to constrain the mass distribution in the galaxy have suggested that at least one additional image…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-12 Jacqueline Chen , Samuel K. Lee , Francisco-Javier Castander , José Maza , Paul L. Schechter

The degeneracy among the disk, bulge and halo contributions to galaxy rotation curves prevents an understanding of the distribution of baryons and dark matter in disk galaxies. In an attempt to break this degeneracy, we present an analysis…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-17 A. A. Dutton , B. J. Brewer , P. J. Marshall , M. W. Auger , T. Treu , D. C. Koo , A. S. Bolton , B. P. Holden , L. V. E. Koopmans

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…

Astrophysics · Physics 2008-11-26 Charles R. Keeton , Joshua N. Winn

We study gravitational lensing by spiral galaxies, using realistic models consisting of halo, disk, and bulge components combined to produce a flat rotation curve. Proper dynamical normalization of the models is critical because a disk…

Astrophysics · Physics 2009-10-30 C. R. Keeton , C. S. Kochanek

We construct a mass model for the spiral lens galaxy 2237+0305, at redshift z_l=0.04, based on gravitational-lensing constraints, HI rotation, and new stellar-kinematic information, based on data taken with the ESI spectrograph on the 10m…

Astrophysics · Physics 2015-05-13 C. M. Trott , T. Treu , L. V. E. Koopmans , R. L. Webster

We determine the mass distribution of a spiral galaxy, 2237+0305 using both gravitational lensing and dynamical constraints. We find that lensing can break the disc-halo degeneracy. 2237+0305 has a sub-maximal disc, contributing 57+/-3 per…

Astrophysics · Physics 2009-11-07 Cathryn M. Trott , Rachel L. Webster

We investigate gravitational lensing by a realistic model of disk galaxies. Most of the mass is contained in a large spherical isothermal dark matter halo, but the potential is modified significantly in the core by a…

Astrophysics · Physics 2009-10-30 Ole Moeller , A. W. Blain

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…

Astrophysics · Physics 2011-05-23 A. O. Jaunsen , J. Hjorth

A recently discovered quadruply-imaged QSO, SDSS J1004+4112 (Inada et al. 2003; Oguri et al. 2004) in the core of a $z=0.68$ galaxy cluster has an unprecedented image separation of ~13''. This lens gives us a unique opportunity to study the…

Astrophysics · Physics 2007-05-23 Liliya L. R. Williams , Prasenjit Saha

We have studied the mass distribution in the lensing galaxy 2237+0305 using constraints from both gravitational lensing and photometric and spectroscopic observations. We find that with sufficient dynamical information we can constrain the…

Astrophysics · Physics 2007-05-23 C. M. Trott , R. L. Webster

We report the discovery of a pair of quasars at $z=1.487$, with a separation of $8\farcs585\pm0\farcs002$. Subaru Telescope infrared imaging reveals the presence of an elliptical and a disk-like galaxy located almost symmetrically between…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 Cristian E. Rusu , Masamune Oguri , Masanori Iye , Naohisa Inada , Issha Kayo , Min-Su Shin , Dominique Sluse , Michael A. Strauss

We report the discovery of the two-image gravitationally lensed quasar SDSS J133222.62+034739.9 (SDSS J1332+0347) with an image separation of Delta_theta=1.14". This system consists of a source quasar at z_s=1.445 and a lens galaxy at…

We investigate the matter distribution of a spiral galaxy with a counter-rotating stellar core, SDSS J1331+3628 (J1331), independently with gravitational lensing and stellar dynamical modelling. By fitting a gravitational potential model to…

Astrophysics of Galaxies · Physics 2016-09-28 Wilma H. Trick , Glenn van de Ven , Aaron A. Dutton

The degeneracy between the disk and the dark matter contribution to galaxy rotation curves remains an important uncertainty in our understanding of disk galaxies. Here we discuss a new method for breaking this degeneracy using gravitational…

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