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As there is a long-standing controversy over the time delay between the two images of the gravitationally lensed quasar FBQ 0951+2635, we combined early and new optical light curves to robustly measure a delay of 13.5 +/- 1.6 d (1sigma…

星系天体物理 · 物理学 2025-02-05 Vyacheslav N. Shalyapin , Luis J. Goicoechea , Eleana Ruiz-Hinojosa

We report the discovery of the two-image gravitationally lensed quasar SDSS J1335+0118. The object was selected as a lens candidate from the Sloan Digital Sky Survey. The imaging and spectroscopic follow-up observations confirm that the…

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

Strongly lensed quasars with time-delay measurements are well known to provide the "time-delay distances" $D_{\Delta t}=(1+z_L)D_LD_S/D_{LS}$ and the angular diameter distances to lens galaxies $D_L$. These two kinds of distances give…

宇宙学与河外天体物理 · 物理学 2019-09-19 Kai Liao

Strong lensing by an isolated spherically symmetric mass distribution is considered in presence of a positive cosmological constant. Deflection angles and time delay are computed and compared to the multiple image of the quasar SDSS…

天体物理学 · 物理学 2008-05-13 Thomas Schucker

We present new brightness monitoring observations of the 4 components of gravitationally lensed system Q2237+0305, which show detection of an intrinsic quasar brightness fluctuation at a time of subdued microlensing activity, between June…

天体物理学 · 物理学 2009-11-11 V. Vakulik , R. Schild , V. Dudinov , S. Nuritdinov , V. Tsvetkova , O. Burkhonov , T. Akhunov

Observed time delays between images of a lensed QSO lead to the determination of the Hubble constant by Refsdal's method, provided the mass distribution in the lensing galaxy is reasonably well known. Since the two or four QSO images…

天体物理学 · 物理学 2009-10-31 Liliya L. R. Williams , Prasenjit Saha

We present a new method for determining time delays among the light curves of various images in a gravitational lens. The method is based on constructing a simple model for the source variation and forming a chi squared measure of the…

天体物理学 · 物理学 2016-08-30 Rennan Barkana

We report the detection of a massive high-redshift cluster of galaxies near the quadruple quasar RX J0911+05, using the LRIS instrument on the Keck-II telescope. The cluster is found to have a mean redshift of <z>=0.7689+/-0.002 and a…

天体物理学 · 物理学 2007-05-23 Jean-Paul Kneib , Judith G. Cohen , Jens Hjorth

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

The distribution of differential time delays \Delta t between images produced by strong gravitational lensing contains information on the mass distributions in the lensing objects as well as on cosmological parameters such as H_0. We derive…

天体物理学 · 物理学 2009-11-07 Masamune Oguri , Atsushi Taruya , Yasushi Suto , Edwin L. Turner

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 a parametric, grid-based lens model for the galaxy cluster MACS J1149.5+2223, concentrating on the properties of the first multiply imaged supernova Refsdal. This model complements our updated light-traces-mass (LTM)…

宇宙学与河外天体物理 · 物理学 2021-09-29 Adi Zitrin

The lensed double QSO 0957+561 has a well-measured time delay and hence is useful for a global determination of H0. Uncertainty in the mass distribution of the lens is the largest source of uncertainty in the derived H0. We investigate the…

天体物理学 · 物理学 2009-10-31 Gary Bernstein , Philippe Fischer

Realizing Refsdal's original idea from 1964, we present estimates of the Hubble constant that are complementary to and potentially competitive with those of other cosmological probes. We use the observed positions of 89 multiple images,…

宇宙学与河外天体物理 · 物理学 2018-06-27 C. Grillo , P. Rosati , S. H. Suyu , I. Balestra , G. B. Caminha , A. Halkola , P. L. Kelly , M. Lombardi , A. Mercurio , S. A. Rodney , T. Treu

We present new measurements of the values of the Hubble constant, matter density, dark energy density, and dark energy density equation-of-state parameters from a full strong lensing analysis of the observed positions of 89 multiple images…

宇宙学与河外天体物理 · 物理学 2024-04-24 C. Grillo , L. Pagano , P. Rosati , S. H. Suyu

We present accurate time delays for the quadruply imaged quasar HE 0435-1223. The delays were measured from 575 independent photometric points obtained in the R-band between January 2004 and March 2010. With seven years of data, we clearly…

宇宙学与河外天体物理 · 物理学 2015-05-19 F. Courbin , V. Chantry , Y. Revaz , D. Sluse , C. Faure , M. Tewes , E. Eulaers , M. Koleva , I. Asfandiyarov , S. Dye , P. Magain , H. van Winckel , J. Coles , P. Saha , M. Ibrahimov , G. Meylan

We report the discovery of a new quadruply imaged quasar surrounded by an optical Einstein ring candidate. Spectra of the different components of 1RXS J113155.4-123155 reveal a source at z=0.658. Up to now, this object is the closest known…

天体物理学 · 物理学 2009-11-10 D. Sluse , J. Surdej , J. -F. Claeskens , D. Hutsemekers , C. Jean , F. Courbin , T. Nakos , M. Billeres , S. V. Khmil

We present an analysis of the properties of the lensing cluster MS0440+0204 at z=0.1965. MS0440+0204 has been observed with a variety of telescopes at diverse wavelengths: from the ground with CFHT, MMT and KECK and from Earth orbit with…

天体物理学 · 物理学 2009-10-30 I. M. Gioia , E. J. Shaya , O. Le Fevre , E. E. Falco , G. A. Luppino , F. Hammer