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相关论文: A Two-Year Time Delay for the Lensed Quasar SDSS J…

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We present 426 epochs of optical monitoring data spanning 1000 days from December 2003 to June 2006 for the gravitationally lensed quasar SDSS J1004+4112. The time delay between the A and B images is 38.4+/-2.0 days in the expected sense…

We report first results from an ongoing monitoring campaign to measure time delays between the six images of the quasar SDSS\,J2222$+$2745, gravitationally lensed by a galaxy cluster. The time delay between A and B, the two most highly…

宇宙学与河外天体物理 · 物理学 2015-11-04 H. Dahle , M. D. Gladders , K. Sharon , M. B. Bayliss , J. R. Rigby

We report the discovery of a cluster-scale lensed quasar, SDSS J1029+2623, selected from the Sloan Digital Sky Survey. The lens system exhibits two lensed images of a quasar at z_s=2.197. The image separation of 22.5" makes it the largest…

We present new light curves for the four bright images of the five image cluster-lensed quasar gravitational lens system SDSS~J1004+4112. The light curves span 14.5 yr and allow measurement of the time delay between the trailing bright…

星系天体物理 · 物理学 2022-09-28 J. A. Muñoz , C. S. Kochanek , J. Fohlmeister , J. Wambsganss , E. Falco , R. Forés-Toribio

We study the geometry and the internal structure of the outflowing wind from the accretion disk of a quasar by observing multiple sightlines with the aid of strong gravitational lensing. Using Subaru/HDS, we performed high-resolution ($R$…

星系天体物理 · 物理学 2015-06-23 Toru Misawa , Naohisa Inada , Masamune Oguri , Poshak Gandhi , Takashi Horiuchi , Suzuka Koyamada , Rina Okamoto

We present 107 new epochs of optical monitoring data for the four brightest images of the gravitational lens SDSS J1004+4112 observed between October 2006 and June 2007. Combining this data with the previously obtained light curves, we…

天体物理学 · 物理学 2009-11-13 J. Fohlmeister , C. S. Kochanek , E. E. Falco , C. W. Morgan , J. Wambsganss

We present results from Chandra observations of the cluster lens SDSS J1029+2623 at z_l=0.58, which is a gravitationally lensed quasar with the largest known image separation. We clearly detect X-ray emission both from the lensing cluster…

We report the discovery of a unique gravitational lens system, SDSSJ2222+2745, producing five spectroscopically confirmed images of a z_s=2.82 quasar lensed by a foreground galaxy cluster at z_l=0.49. We also present photometric and…

We analyse new optical observations of the gravitational lens system SDSS J1515+1511. These include a 2.6-year photometric monitoring with the Liverpool Telescope (LT) in the $r$ band, as well as a spectroscopic follow-up with the LT and…

星系天体物理 · 物理学 2017-02-15 Vyacheslav N. Shalyapin , Luis J. Goicoechea

We study the origin of absorption features on the blue side of the C IV broad emission line of the large-separation lensed quasar SDSS J1029+2623 at z_em ~ 2.197. The quasar images, produced by a foreground cluster of galaxies, have a…

宇宙学与河外天体物理 · 物理学 2015-06-12 Toru Misawa , Naohisa Inada , Ken Ohsuga , Poshak Gandhi , Rohta Takahashi , Masamune Oguri

We have measured the time delay between the two images of the gravitationally lensed quasar HE1104-1805 by combining observations made with the Wise Observatory 1m telescope and published observations of this system by Schechter et al.,…

天体物理学 · 物理学 2009-11-07 Eran O. Ofek , Dan Maoz

This paper presents optical R-band light curves and the time delay of the doubly imaged gravitationally lensed quasar SDSS J1001+5027 at a redshift of 1.838. We have observed this target for more than six years, between March 2005 and July…

宇宙学与河外天体物理 · 物理学 2013-08-29 S. Rathna Kumar , M. Tewes , C. S. Stalin , F. Courbin , I. Asfandiyarov , G. Meylan , E. Eulaers , T. P. Prabhu , P. Magain , H. Van Winckel , Sh. Ehgamberdiev

We present optical lightcurves of the gravitationally lensed components A (=A1+A2+A3) and B of the quadruple quasar RX J0911.4+0551 (z = 2.80). The observations were primarily obtained at the Nordic Optical Telescope between 1997 March and…

SDSS J2222+2745 is a galaxy cluster at z=0.49, strongly lensing a quasar at z=2.805 into six widely separated images. In recent HST imaging of the field, we identify additional multiply lensed galaxies, and confirm the sixth quasar image…

We have built a new model for the lens system SDSS J1004+4112 including the recently measured time delay of the fourth quasar image. This time delay has a strong influence on the inner mass distribution of the lensing cluster ($\rho \propto…

星系天体物理 · 物理学 2022-09-28 R. Forés-Toribio , J. A. Muñoz , C. S. Kochanek , E. Mediavilla

We spectroscopically re-observed the gravitational lens system SDSS J1339+1310 using OSIRIS on the GTC. We also monitored the $r$-band variability of the two quasar images (A and B) with the LT over 143 epochs in the period 2009$-$2016.…

星系天体物理 · 物理学 2016-12-07 Luis J. Goicoechea , Vyacheslav N. Shalyapin

We report that the Sloan Digital Sky Survey quasar SDSS J165043.44+425149.3 is gravitationally lensed into two images, based on observations obtained with the WIYN 3.5 m telescope at the Kitt Peak National Observatory. The lensed quasar, at…

天体物理学 · 物理学 2016-08-30 Nicholas D. Morgan , Jeffrey A. Snyder , Louis H. Reens

We present the results from nine years of optically monitoring the gravitationally lensed z=0.658 quasar RX J1131-1231. The R-band light curves of the four individual images of the quasar were obtained using deconvolution photometry for a…

宇宙学与河外天体物理 · 物理学 2015-06-11 M. Tewes , F. Courbin , G. Meylan , C. S. Kochanek , E. Eulaers , N. Cantale , A. M. Mosquera , P. Magain , H. Van Winckel , D. Sluse , G. Cataldi , D. Voros , S. Dye

Aims: Our aim is to measure the time delay between the two gravitationally lensed images of the z = 1.547 quasar SDSS J1650+4251, in order to estimate the Hubble constant H_0. Methods: Our measurement is based on R-band light curves with 57…

We present a strong lensing analysis of the galaxy cluster SDSS J1029+2623 at $z=0.588$, one of the few currently known lens clusters with multiple images of a background ($z=2.1992$) quasar with a measured time delay. We use archival…

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