Paper
Gaia GraL X.: The GraL catalogue of gravitationally lensed quasars Matched with \textit{Gaia} data, redshifts, and time delays
Authors
C. Ducourant, R. Teixeira, P. H. Vale-Cunha, L. Delchambre, A. Krone-Martins, J. Braine, L. Galluccio, J-F. Le Campion, O. S. Krinski-Moreira, S. Scarano, C. Boehm, T. Connor, S. G. Djorgovski, M. J. Graham, P. Jalan, Q. Petit, S. A. Klioner, F. Mignard, V. Negi, J. Sebastian den Brok, I. Slezak, E. Slezak, C. Spindola-Duarte, D. Stern, J. Surdej, D. Sweeney, D. J. Walton, J. Wambsganss
Abstract
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 confirmed lensed quasars with ESA/{\it Gaia} astrometry and photometry, as well as redshifts and time delays when available. In addition to the improved astrometry, the catalogue increases the number of lensed quasars by a factor of 1.5 (now 364, of which 277 are doubles and 87 are quads or triples) and significantly increases the number of lensing galaxies detected (now 218), which represents a major step forward. Redshifts are provided for 347 quasars and 188 deflectors. A completely new table of time delays, required for estimates of $H_0$, is presented, with 195 time delays from 73 systems. {\it Gaia} absolute astrometry is sub-milliarcsecond and covers the entire sky. Future {\it Gaia} data releases will provide long-term photometry, which should provide many more time delays. The catalogues as presented here enable machine-learning techniques to be trained and tested and subsequently applied to the {\it Gaia} data releases. Finally, we derive simple but homogeneous models of the 18 quadruply imaged quasars for which images of all four components are presented in {\it Gaia} DR3.}
Metadata
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Raw Data (Debug)
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"raw_xml": "<entry>\n <id>http://arxiv.org/abs/2603.12810v1</id>\n <title>Gaia GraL X.: The GraL catalogue of gravitationally lensed quasars Matched with \\textit{Gaia} data, redshifts, and time delays</title>\n <updated>2026-03-13T09:12:23Z</updated>\n <link href='https://arxiv.org/abs/2603.12810v1' rel='alternate' type='text/html'/>\n <link href='https://arxiv.org/pdf/2603.12810v1' rel='related' title='pdf' type='application/pdf'/>\n <summary>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 confirmed lensed quasars with ESA/{\\it Gaia} astrometry and photometry, as well as redshifts and time delays when available. In addition to the improved astrometry, the catalogue increases the number of lensed quasars by a factor of 1.5 (now 364, of which 277 are doubles and 87 are quads or triples) and significantly increases the number of lensing galaxies detected (now 218), which represents a major step forward. Redshifts are provided for 347 quasars and 188 deflectors. A completely new table of time delays, required for estimates of $H_0$, is presented, with 195 time delays from 73 systems. {\\it Gaia} absolute astrometry is sub-milliarcsecond and covers the entire sky. Future {\\it Gaia} data releases will provide long-term photometry, which should provide many more time delays. The catalogues as presented here enable machine-learning techniques to be trained and tested and subsequently applied to the {\\it Gaia} data releases. Finally, we derive simple but homogeneous models of the 18 quadruply imaged quasars for which images of all four components are presented in {\\it Gaia} DR3.}</summary>\n <category scheme='http://arxiv.org/schemas/atom' term='astro-ph.GA'/>\n <category scheme='http://arxiv.org/schemas/atom' term='astro-ph.CO'/>\n <published>2026-03-13T09:12:23Z</published>\n <arxiv:primary_category term='astro-ph.GA'/>\n <author>\n <name>C. Ducourant</name>\n </author>\n <author>\n <name>R. Teixeira</name>\n </author>\n <author>\n <name>P. H. Vale-Cunha</name>\n </author>\n <author>\n <name>L. Delchambre</name>\n </author>\n <author>\n <name>A. Krone-Martins</name>\n </author>\n <author>\n <name>J. Braine</name>\n </author>\n <author>\n <name>L. Galluccio</name>\n </author>\n <author>\n <name>J-F. Le Campion</name>\n </author>\n <author>\n <name>O. S. Krinski-Moreira</name>\n </author>\n <author>\n <name>S. Scarano</name>\n </author>\n <author>\n <name>C. Boehm</name>\n </author>\n <author>\n <name>T. Connor</name>\n </author>\n <author>\n <name>S. G. Djorgovski</name>\n </author>\n <author>\n <name>M. J. Graham</name>\n </author>\n <author>\n <name>P. Jalan</name>\n </author>\n <author>\n <name>Q. Petit</name>\n </author>\n <author>\n <name>S. A. Klioner</name>\n </author>\n <author>\n <name>F. Mignard</name>\n </author>\n <author>\n <name>V. Negi</name>\n </author>\n <author>\n <name>J. Sebastian den Brok</name>\n </author>\n <author>\n <name>I. Slezak</name>\n </author>\n <author>\n <name>E. Slezak</name>\n </author>\n <author>\n <name>C. Spindola-Duarte</name>\n </author>\n <author>\n <name>D. Stern</name>\n </author>\n <author>\n <name>J. Surdej</name>\n </author>\n <author>\n <name>D. Sweeney</name>\n </author>\n <author>\n <name>D. J. Walton</name>\n </author>\n <author>\n <name>J. Wambsganss</name>\n </author>\n </entry>"
}