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This is the first version (v1) of the Gravitational LENses and DArk MAtter (GLENDAMA) database accessible at http://grupos.unican.es/glendama/database The new database contains more than 6000 ready-to-use (processed) astronomical frames…

天体物理仪器与方法 · 物理学 2015-05-20 Luis J. Goicoechea , Vyacheslav N. Shalyapin , Rodrigo Gil-Merino

A gravitational lens (GL)-search program, initiated in 1990 at the Nordic Optical Telescope (NOT), has revealed several possible GL-candidates among a sample of 168 quasars (QSOs), chosen from three lists compiled by C. Hazard, D. Reimers…

天体物理学 · 物理学 2016-08-30 A. O. Jaunsen , M. Jablonski , B. R. Pettersen , R. Stabell

We present the overview and current results of an ongoing optical/NIR monitoring of seven GLQs with the 2-m Liverpool Robotic Telescope. The photometric data over the first seven years of this programme (2005-2011) are leading to…

星系天体物理 · 物理学 2015-06-03 Luis J. Goicoechea , Vyacheslav N. Shalyapin

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…

Context. Strong gravitationally lensed quasars are among the most interesting and useful observable extragalactic phenomena. Because their study constitutes a unique tool in various fields of astronomy, they are highly sought, not without…

We present XMM-Newton X-ray observations of nine confirmed lensed quasars at $1 \lesssim z \lesssim 3$ identified by the Gaia Gravitational Lens program. Eight systems are strongly detected, with 0.3--8.0 keV fluxes $F_{0.3-8.0} \gtrsim 5…

We report the discovery and spectroscopic confirmation of 22 new gravitationally lensed quasars found using $\textit{Gaia}$ data release 2. The selection was made using several techniques: multiple $\textit{Gaia}$ detections around objects…

星系天体物理 · 物理学 2019-01-11 Cameron A. Lemon , Matthew W. Auger , Richard G. McMahon

Gravitationally-lensed quasars can be discovered as a by-product of galaxy redshift surveys. Lenses discovered spectroscopically in this way should require less observational effort per event than those found in dedicated lens surveys.…

天体物理学 · 物理学 2009-10-31 Daniel J. Mortlock , Rachel L. Webster

Gravitational lensing is a powerful tool for the study of the distribution of dark matter in the Universe. The cold-dark-matter model of the formation of large-scale structures predicts the existence of quasars gravitationally lensed by…

We report the final results of the search for gravitationally lensed flat-spectrum radio sources found in the combination of CLASS (Cosmic Lens All Sky Survey) and JVAS (Jodrell-Bank VLA Astrometric Survey). VLA observations of 16,503…

Gravitationally lensed quasars (GLQs) are known to potentially provide an independent way of determining the value of the Hubble-Lema\^{i}tre parameter $H_{0}$, to probe the dark matter content of lensing galaxies and to resolve tiny…

Context. Strongly lensed quasars are fundamental sources for cosmology. The Gaia space mission covers the entire sky with the unprecedented resolution of $0.18$" in the optical, making it an ideal instrument to search for gravitational…

星系天体物理 · 物理学 2024-05-22 Gaia Collaboration , A. Krone-Martins , C. Ducourant , L. Galluccio , L. Delchambre , I. Oreshina-Slezak , R. Teixeira , J. Braine , J. -F. Le Campion , F. Mignard , W. Roux , A. Blazere , L. Pegoraro , A. G. A. Brown , A. Vallenari , T. Prusti , J. H. J. de Bruijne , F. Arenou , C. Babusiaux , A. Barbier , M. Biermann , O. L. Creevey , D. W. Evans , L. Eyer , R. Guerra , A. Hutton , C. Jordi , S. A. Klioner , U. Lammers , L. Lindegren , X. Luri , S. Randich , P. Sartoretti , R. Smiljanic , P. Tanga , N. A. Walton , C. A. L. Bailer-Jones , U. Bastian , M. Cropper , R. Drimmel , D. Katz , C. Soubiran , F. van Leeuwen , M. Audard , J. Bakker , R. Blomme , J. Castaneda , F. De Angeli , C. Fabricius , M. Fouesneau , Y. Fremat , A. Guerrier , E. Masana , R. Messineo , C. Nicolas , K. Nienartowicz , F. Pailler , P. Panuzzo , F. Riclet , G. M. Seabroke , R. Sordo , F. Thevenin , G. Gracia-Abril , J. Portell , D. Teyssier , M. Altmann , K. Benson , J. Berthier , P. W. Burgess , D. Busonero , G. Busso , H. Canovas , B. Carry , N. Cheek , G. Clementini , Y. Damerdji , M. Davidson , P. de Teodoro , A. Dell'Oro , E. Fraile Garcia , D. Garabato , P. Garcia-Lario , N. Garralda Torres , P. Gavras , R. Haigron , N. C. Hambly , D. L. Harrison , D. Hatzidimitriou , J. Hernandez , S. T. Hodgkin , B. Holl , S. Jamal , S. Jordan , A. C. Lanzafame , W. Loffler , A. Lorca , O. Marchal , P. M. Marrese , A. Moitinho , K. Muinonen , M. Nunez Campos , P. Osborne , E. Pancino , T. Pauwels , A. Recio-Blanco , M. Riello , L. Rimoldini , A. C. Robin , T. Roegiers , L. M. Sarro , M. Schultheis , C. Siopis , M. Smith , A. Sozzetti , E. Utrilla , M. van Leeuwen , K. Weingrill , U. Abbas , P. Abraham , A. Abreu Aramburu , C. Aerts , G. Altavilla , M. A. Alvarez , J. Alves , R. I. Anderson , T. Antoja , D. Baines , S. G. Baker , Z. Balog , C. Barache , D. Barbato , M. Barros , M. A. Barstow , S. Bartolome , D. Bashi , N. Bauchet , N. Baudeau , U. Becciani , L. R. Bedin , I. Bellas-Velidis , M. Bellazzini , W. Beordo , A. Berihuete , M. Bernet , C. Bertolotto , S. Bertone , L. Bianchi , A. Binnenfeld , T. Boch , A. Bombrun , S. Bouquillon , A. Bragaglia , L. Bramante , E. Breedt , A. Bressan , N. Brouillet , E. Brugaletta , B. Bucciarelli , A. G. Butkevich , R. Buzzi , E. Caffau , R. Cancelliere , S. Cannizzo , R. Carballo , T. Carlucci , M. I. Carnerero , J. M. Carrasco , J. Carretero , S. Carton , L. Casamiquela , M. Castellani , A. Castro-Ginard , V. Cesare , P. Charlot , L. Chemin , V. Chiaramida , A. Chiavassa , N. Chornay , R. Collins , G. Contursi , W. J. Cooper , T. Cornez , M. Crosta , C. Crowley , C. Dafonte , P. de Laverny , F. De Luise , R. De March , R. de Souza , A. de Torres , E. F. del Peloso , M. Delbo , A. Delgado , T. E. Dharmawardena , S. Diakite , C. Diener , E. Distefano , C. Dolding , K. Dsilva , J. Duran , H. Enke , P. Esquej , C. Fabre , M. Fabrizio , S. Faigler , M. Fatovic , G. Fedorets , J. Fernandez-Hernandez , P. Fernique , F. Figueras , Y. Fournier , C. Fouron , M. Gai , M. Galinier , A. Garcia-Gutierrez , M. Garcia-Torres , A. Garofalo , E. Gerlach , R. Geyer , P. Giacobbe , G. Gilmore , S. Girona , G. Giuffrida , R. Gomel , A. Gomez , J. Gonzalez-Nunez , I. Gonzalez-Santamaria , E. Gosset , M. Granvik , V. Gregori Barrera , R. Gutierrez-Sanchez , M. Haywood , A. Helmer , A. Helmi , K. Henares , S. L. Hidalgo , T. Hilger , D. Hobbs , C. Hottier , H. E. Huckle , M. Jablonska , F. Jansen , O. Jimenez-Arranz , J. Juaristi Campillo , S. Khanna , G. Kordopatis , A. Kospal , Z. Kostrzewa-Rutkowska , M. Kun , S. Lambert , A. F. Lanza , Y. Lebreton , T. Lebzelter , S. Leccia , I. Lecoeur-Taibi , G. Lecoutre , S. Liao , L. Liberato , E. Licata , H. E. P. Lindstrom , T. A. Lister , E. Livanou , A. Lobel , C. Loup , L. Mahy , R. G. Mann , M. Manteiga , J. M. Marchant , M. Marconi , D. Marin Pina , S. Marinoni , D. J. Marshall , J. Martin Lozano , J. M. Martin-Fleitas , G. Marton , N. Mary , A. Masip , D. Massari , A. Mastrobuono-Battisti , T. Mazeh , P. J. McMillan , J. Meichsner , S. Messina , D. Michalik , N. R. Millar , A. Mints , D. Molina , R. Molinaro , L. Molnar , G. Monari , M. Monguio , P. Montegriffo , A. Montero , R. Mor , A. Mora , R. Morbidelli , T. Morel , D. Morris , N. Mowlavi , D. Munoz , T. Muraveva , C. P. Murphy , I. Musella , Z. Nagy , S. Nieto , L. Noval , A. Ogden , C. Ordenovic , C. Pagani , I. Pagano , L. Palaversa , P. A. Palicio , L. Pallas-Quintela , A. Panahi , C. Panem , S. Payne-Wardenaar , A. Penttila , P. Pesciullesi , A. M. Piersimoni , M. Pinamonti , F. -X. Pineau , E. Plachy , G. Plum , E. Poggio , D. Pourbaix , A. Prsa , L. Pulone , E. Racero , M. Rainer , C. M. Raiteri , P. Ramos , M. Ramos-Lerate , M. Ratajczak , P. Re Fiorentin , S. Regibo , C. Reyle , V. Ripepi , A. Riva , H. -W. Rix , G. Rixon , N. Robichon , C. Robin , M. Romero-Gomez , N. Rowell , F. Royer , D. Ruz Mieres , K. A. Rybicki , G. Sadowski , A. Saez Nunez , A. Sagrista Selles , J. Sahlmann , V. Sanchez Gimenez , N. Sanna , R. Santovena , M. Sarasso , C. Sarrate Riera , E. Sciacca , J. C. Segovia , D. Segransan , S. Shahaf , A. Siebert , L. Siltala , E. Slezak , R. L. Smart , O. N. Snaith , E. Solano , F. Solitro , D. Souami , J. Souchay , L. Spina , E. Spitoni , F. Spoto , L. A. Squillante , I. A. Steele , H. Steidelmuller , J. Surdej , L. Szabados , F. Taris , M. B. Taylor , K. Tisanic , L. Tolomei , F. Torra , G. Torralba Elipe , M. Trabucchi , M. Tsantaki , A. Ulla , N. Unger , O. Vanel , A. Vecchiato , D. Vicente , S. Voutsinas , M. Weiler , L. Wyrzykowski , H. Zhao , J. Zorec , T. Zwitter , L. Balaguer-Nunez , N. Leclerc , S. Morgenthaler , G. Robert , S. Zucker

We present a mock catalog of gravitationally lensed quasars at $z_\text{qso}<7.5$ with simulated images for the Rubin Observatory Legacy Survey of Space and Time (LSST). We adopt recent measurements of quasar luminosity functions to model…

星系天体物理 · 物理学 2022-03-02 Minghao Yue , Xiaohui Fan , Jinyi Yang , Feige Wang

We argue that globular clusters (GCs) are good candidates for gravitational lenses in explaining quasar-galaxy associations. The catalog of associations (Bukhmastova 2001) compiled from the LEDA catalog of galaxies (Paturel 1997) and from…

天体物理学 · 物理学 2009-11-07 Yu. L. Bukhmastova

Gravitational lens systems containing lensed quasars are important as cosmological probes, as diagnostics of structural properties of the lensing galaxies and as tools to study the quasars themselves. The largest lensed quasar sample is the…

宇宙学与河外天体物理 · 物理学 2015-05-30 Neal Jackson , Hayden Rampadarath , Eran O. Ofek , Masamune Oguri , Min-Su Shin

We present a pipeline to identify photometric variability within strong gravitationally lensing candidates, in the DESI Legacy Imaging Surveys. In our first paper (Sheu et al. 2023), we laid out our pipeline and presented seven new…

We have conducted a search for strong gravitational lensing systems in the Dark Energy Spectroscopic Instrument (DESI) Legacy Imaging Surveys Data Release 9. This is the third paper in a series. These surveys together cover $\sim$19,000…

Cadenced optical imaging surveys in the next decade will be capable of detecting time-varying galaxy-scale strong gravitational lenses in large numbers, increasing the size of the statistically well-defined samples of multiply-imaged…

宇宙学与河外天体物理 · 物理学 2015-05-14 Masamune Oguri , Philip J. Marshall

We report the discovery of a new gravitationally lensed quasar (double) from the Optical Gravitational Lensing Experiment (OGLE) identified inside the $\sim$670 sq. deg area encompassing the Magellanic Clouds. The source was selected as one…

Determining the Hubble constant tension requires alternative strategies, and multiply imaged quasars, with their intermediate redshifts, can potentially be used in this regard. We provide a currently complete catalogue of spectroscopically…

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