Astrophysics - Instrumentation and Methods for Astrophysics; Astrophysics - Astrophysics of Galaxies
Abstract :
[en] Thanks to its spatial resolution the ESA/Gaia space mission offers a unique opportunity to discover new multiply-imaged quasars and to study the already known lensed systems at sub-milliarcsecond astrometric precisions. In this paper, we address the detection of the known multiply-imaged quasars from the Gaia Data Release 2 and determine the astrometric and photometric properties of the individually detected images found in the Gaia DR2 catalogue. We have compiled an exhaustive list of quasar gravitational lenses from the literature to search for counterparts in the Gaia Data Release 2. We then analyze the astrometric and photometric properties of these Gaia's detections. To highlight the tremendous potential of Gaia at the sub-milliarcsecond level we finally perform a simple Bayesian modeling of the well-known gravitational lens system HE0435-1223, using Gaia Data Release 2 and HST astrometry. From 478 known multiply imaged quasars, 200 have at least one image found in the Gaia Data Release 2. Among the 41 known quadruply-imaged quasars of the list, 26 have at least one image in the Gaia Data Release 2, 12 of which are fully detected, 6 have three counterparts, 7 have two and 1 has only one. As expected, the modeling of HE0435-1223 shows that the model parameters are significantly better constrained when using Gaia astrometry compared to HST astrometry, in particular the relative positions of the background quasar source and the centroid of the deflector. The Gaia sub-milliarcsecond astrometry also significantly reduces the parameter correlations. Besides providing an up-to-date list of multiply imaged quasars and their detection in the Gaia DR2, this paper shows that more complex modeling scenarios will certainly benefit from Gaia sub-milliarcsecond astrometry.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Ducourant, C.; Laboratoire d'Astrophysique de Bordeaux, Univ. Bordeaux, CNRS, B18N, allée Geoffroy Saint-Hilaire, 33615, Pessac, France
Wertz, O.; Argelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, 53121, Bonn, Germany
Krone-Martins, A.; CENTRA, Faculdade de Ciências, Universidade de Lisboa, Ed. C8, Campo Grande, 1749-016, Lisboa, Portugal
Teixeira, R.; Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, Rua do Matão, 1226, Cidade Universitária, 05508-900, São Paulo, SP, Brazil
Le Campion, J.-F.; Laboratoire d'Astrophysique de Bordeaux, Univ. Bordeaux, CNRS, B18N, allée Geoffroy Saint-Hilaire, 33615, Pessac, France
Galluccio, L.; Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Boulevard de l'Observatoire, CS 34229, 06304 Nice, France
Klüter, J.; Zentrum für Astronomie der Universität Heidelberg, Astronomisches Rechen-Institut, Mönchhofstr. 12-14, 69120, Heidelberg, Germany
Delchambre, Ludovic ; Université de Liège - ULiège > Groupe d'astrophysique des hautes énergies (GAPHE)
Surdej, Jean ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Département d'astrophys., géophysique et océanographie (AGO)
Mignard, F.; Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Boulevard de l'Observatoire, CS 34229, 06304 Nice, France
Wambsganss, J.; Zentrum für Astronomie der Universität Heidelberg, Astronomisches Rechen-Institut, Mönchhofstr. 12-14, 69120, Heidelberg, Germany ; International Space Science Institute (ISSI), Hallerstraße 6, 3012, Bern, Switzerland
Bastian, U.; Zentrum für Astronomie der Universität Heidelberg, Astronomisches Rechen-Institut, Mönchhofstr. 12-14, 69120, Heidelberg, Germany
Graham, M. J.; California Institute of Technology, 1200 E. California Blvd, Pasadena, CA 91125, USA
Djorgovski, S. G.; California Institute of Technology, 1200 E. California Blvd, Pasadena, CA 91125, USA
Slezak, E.; Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Boulevard de l'Observatoire, CS 34229, 06304 Nice, France)
Hartley, P., Flamary, R., Jackson, N., Tagore, A. S., & Metcalf, R. B. 2017, MNRAS, 471, 3378
Hobbs, D., Høg, E., & Mora, A. 2016,. ArXiv e-prints [arXiv:1609.07325].
Huchra, J., Gorenstein, M., Kent, S., et al. 1985, AJ, 90, 691
Inada, N., Becker, R.H., & Burles, S. 2003 a, AJ, 126, 666
Inada, N., Oguri, M., Pindor, B., et al. 2003 b, Nature, 426, 810
Inada, N., Burles, S., Gregg, M. D., et al. 2005, AJ, 130, 1967
Inada, N., Oguri, M., Becker, R. H., et al. 2006, AJ, 131, 1934
Inada, N., Oguri, M., Becker, R. H., et al. 2007, AJ, 133, 206
Inada, N., Oguri, M., Shin, M.-S., et al. 2010, AJ, 140, 403
Inada, N., Oguri, M., Shin, M.-S., et al. 2012, AJ, 143, 119
Inada, N., Oguri, M., Rusu, C. E., Kayo, I., & Morokuma, T. 2014, AJ, 147, 153
Jackson, N. 2008, MNRAS, 389, 1311
Jackson, N., Rampadarath, H., Ofek, E. O., Oguri, M., & Shin, M.-S. 2012, MNRAS, 419, 2014
Johnston, D. E., Richards, G. T., Frieman, J. A., et al. 2003, AJ, 126, 2281
Keeton, C. R., 2001, ApJ,. submitted [arXiv:astro-ph/0102340]
Keeton, C. R. 2010, Gen. Relativ. Gravit., 42, 2151
Kochanek, C. S. 2006, Gravitational Lensing: Strong, Weak and Micro, eds. G. Meylan P. Jetzer P. North, et al. Saas-Fee Advanced Course 33, 91
Kochanek, C. S., Falco, E. E., & Impey, C. D. 1999, in After the Dark Ages: When Galaxies were Young, eds. S. Holt, & E. Smith, AIP Conf. Ser., 470, 163
Kochanek, C. S., Morgan, N. D., Falco, E. E., et al. 2006, ApJ, 640, 47
Kormann, R., Schneider, P., & Bartelmann, M. 1994, A&A, 284, 285