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相关论文: Microlensing Analysis for the gravitational lens s…

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We present a multi-wavelength study of the gravitational lens COSMOS J095930+023427 (z=0.89), together with the associated galaxy group located at $z\sim0.7$ along the line of sight and the lensed background galaxy. The source redshift is…

宇宙学与河外天体物理 · 物理学 2015-06-12 Shuo Cao , Giovanni Covone , Maurizio Paolillo , Zong-Hong Zhu

We estimate the fraction of mass that is composed of compact objects in gravitational lens galaxies. This study is based on microlensing measurements (obtained from the literature) of a sample of 29 quasar image pairs seen through 20 lens…

宇宙学与河外天体物理 · 物理学 2014-11-20 E. Mediavilla , J. A. Munoz , E. Falco , V. Motta , E. Guerras , H. Canovas , C. Jean , A. Oscoz , A. M. Mosquera

We present an $r$--band photometric monitoring of the two images A and B of the gravitationally lensed quasar SDSS J1442+4055 using the Liverpool Telescope (LT). From the LT light curves between 2015 December and 2018 August, we derive at…

星系天体物理 · 物理学 2019-03-18 Vyacheslav N. Shalyapin , Luis J. Goicoechea

We analyze V, I and H band HST images and two seasons of R-band monitoring data for the gravitationally lensed quasar SDSS0924+0219. We clearly see that image D is a point-source image of the quasar at the center of its host galaxy. We can…

天体物理学 · 物理学 2011-02-11 Christopher W. Morgan , C. S. Kochanek , Nicholas D. Morgan , Emilio E. Falco

Direct measurements of dark matter distributions in galaxies are currently only possible through the use of gravitational lensing observations. Combinations of lens modelling and stellar velocity dispersion measurements provide the best…

宇宙学与河外天体物理 · 物理学 2015-05-27 N. F. Bate , D. J. E. Floyd , R. L. Webster , J. S. B. Wyithe

We aim to reveal the sizes of the continuum and broad emission line (BEL) emitting regions in the gravitationally lensed quasar SDSS J1004+4112 by analyzing the unique signatures of microlensing in this system. Through a comprehensive…

Using a sample of almost 7000 strong MgII absorbers with 0.4 < z < 2.2 detected in the SDSS DR4 dataset, we investigate the gravitational lensing and dust extinction effects they induce on background quasars. After carefully quantifying…

天体物理学 · 物理学 2009-11-13 Brice Ménard , Daniel Nestor , David Turnshek , Anna Quider , Gordon Richards , Doron Chelouche , Sandhya Rao , ;

We present detailed maps of the microlensing optical depth and event density over an area of 195 sq. deg towards the Galactic bulge. The maps are computed from synthetic stellar catalogues generated from the Besancon Galaxy Model, which…

天体物理学 · 物理学 2015-05-13 E. Kerins , A. C. Robin , D. J. Marshall

We present evidence for ultraviolet/optical microlensing in the gravitationally lensed quasar Q0957+561. We combine new measurements from our optical monitoring campaign at the United States Naval Observatory, Flagstaff (USNO) with…

We predict the effects of gravitational lensing on the color-selected flux-limited samples of z~4.3 and z>5.8 quasars, recently published by the Sloan Digital Sky Survey (SDSS). Our main findings are: (i) The lensing probability should be…

天体物理学 · 物理学 2009-11-07 Stuart Wyithe , Abraham Loeb

We present Submillimeter Array observations of the z=3.91 gravitationally lensed broad absorption line quasar APM08279+5255 which spatially resolve the 1.0mm (0.2mm rest-frame) dust continuum emission. At 0.4" resolution, the emission is…

天体物理学 · 物理学 2009-11-13 M. Krips , A. B. Peck , K. Sakamoto , G. B. Petitpas , D. J. Wilner , S. Matsushita , D. Iono

We analyzed Chandra observations of three gravitational lenses, SBS0909+523, FBQS0951+2635, and B1152+199, to measure the differential X-ray absorption and the dust-to-gas ratio of the lens galaxies. We successfully detected the…

天体物理学 · 物理学 2009-06-23 Xinyu Dai , Christopher S. Kochanek

We investigate reddening by Milky Way dust in the low-extinction regime of $E_{B-V}<0.15$. Using over 50,000 QSOs at $0.5<z<2.5$ from the SDSS DR7 QSO Catalogue we probe the residual SDSS colours after dereddening and correcting for the…

星系天体物理 · 物理学 2015-06-23 Christian Wolf

The objective of this work is to obtain an extinction-corrected distribution of optical surface brightness and colour indices of the large nearby galaxy M 31 using homogeneous observational data and a model for intrinsic extinction. We…

宇宙学与河外天体物理 · 物理学 2011-03-14 Elmo Tempel , Taavi Tuvikene , Antti Tamm , Peeter Tenjes

Context. The gravitational lens system SDSS J1004+4112 was the first known example of a quasar lensed by a galaxy cluster. The interest in this system has been renewed following the publication of r-band light curves spanning 14.5 years and…

星系天体物理 · 物理学 2024-10-10 R. Forés-Toribio , J. A. Muñoz , C. Fian , J. Jiménez-Vicente , E. Mediavilla

Gravitational microlensing is a powerful tool for probing the inner structure of distant quasars. In this context, we have obtained spectropolarimetric observations of the two images of the broad absorption line (BAL) quasar…

星系天体物理 · 物理学 2020-01-22 D. Hutsemékers , D. Sluse , P. Kumar

We consider the influence of (milli/micro)lensing on the spectra of lensed QSOs. We propose a method for the observational detection of microlensing in the spectra of lensed QSOs and apply it to the spectra of the three lensed QSOs (PG…

天体物理学 · 物理学 2009-11-10 L. C. Popovic , G. Chartas

We use single-epoch spectroscopy of three gravitationally lensed quasars, HE0435-1223, WFI2033-4723, and HE2149-2745, to study their inner structure (BLR and continuum source). We detect microlensing-induced magnification in the wings of…

星系天体物理 · 物理学 2017-03-02 V. Motta , E. Mediavilla , K. Rojas , E. E. Falco , J. Jimenez-Vicente , J. A. Munoz

We homogeneously analyzed the \chandra\ X-ray observations of 10 gravitational lenses, HE 0047-1756, QJ 0158-4325, SDSS 0246-0805, HE 0435-1223, SDSS 0924+0219, SDSS 1004+4112, HE 1104-1805, PG 1115+080, Q 1355-2257, and Q 2237+0305, to…

宇宙学与河外天体物理 · 物理学 2013-06-04 Bin Chen , Xinyu Dai , Christopher S. Kochanek , George Chartas

We present narrowband images of the gravitational lens system Q~2237+0305 made with the Nordic Optical Telescope in eight different filters covering the wavelength interval 3510-8130 \AA. Using point-spread function photometry fitting we…

天体物理学 · 物理学 2011-02-11 A. M. Mosquera , J. A. Muñoz , E. Mediavilla