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dc.contributor.authorSTERN, D.
dc.contributor.authorDJORGOVSKI, S. G.
dc.contributor.authorKRONE-MARTINS, A.
dc.contributor.authorSLUSE, D.
dc.contributor.authorDELCHAMBRE, L.
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorDUCOURANT, C.
dc.contributor.authorTEIXEIRA, R.
dc.contributor.authorSURDEJ, J.
dc.contributor.authorBOEHM, C.
dc.contributor.authorBROK, J. Den
dc.contributor.authorDOBIE, D.
dc.contributor.authorDRAKE, A.
hal.structure.identifierJoseph Louis LAGRANGE [LAGRANGE]
dc.contributor.authorGALLUCCIO, Laurent
dc.contributor.authorGRAHAM, M. J.
dc.contributor.authorJALAN, P.
dc.contributor.authorKLARK, J.
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorLECAMPION, J. F.
dc.contributor.authorMAHABAL, A.
hal.structure.identifierJoseph Louis LAGRANGE [LAGRANGE]
dc.contributor.authorMIGNARD, F.
dc.contributor.authorMURPHY, T.
dc.contributor.authorNIERENBERG, A.
dc.contributor.authorSCARANO, S.
dc.contributor.authorSIMON, J.
hal.structure.identifierJoseph Louis LAGRANGE [LAGRANGE]
dc.contributor.authorSLEZAK, E.
dc.contributor.authorSPINDOLA-DUARTE, C.
dc.contributor.authorWAMBSGANSS, J.
dc.date.issued2021-11-01
dc.identifier.issn0004-637X
dc.description.abstractEnCombining the exquisite angular resolution of Gaia with optical light curves and WISE photometry, the Gaia Gravitational Lenses group (GraL) uses machine learning techniques to identify candidate strongly lensed quasars, and has confirmed over two dozen new strongly lensed quasars from the Gaia Data Release 2. This paper reports on the 12 quadruply-imaged quasars identified by this effort to date, which is approximately a 20% increase in the total number of confirmed quadruply-imaged quasars. We discuss the candidate selection, spectroscopic follow-up, and lens modeling. We also report our spectroscopic failures as an aid for future investigations.
dc.language.isoen
dc.publisherAmerican Astronomical Society
dc.title.enGaia GraL: Gaia DR2 Gravitational Lens Systems. VI. Spectroscopic Confirmation and Modeling of Quadruply-Imaged Lensed Quasars
dc.typeArticle de revue
dc.identifier.doi10.3847/1538-4357/ac0f04
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]
dc.identifier.arxiv2012.10051
bordeaux.journalThe Astrophysical Journal
bordeaux.peerReviewedoui
hal.identifierhal-03227284
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-03227284v1
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