Gaia GraL: Gaia DR2 gravitational lens systems – VIII. A radio census of lensed systems

Author:

Dobie Dougal12ORCID,Sluse Dominique3,Deller Adam12ORCID,Murphy Tara24ORCID,Krone-Martins Alberto56,Stern Daniel7,Wang Ziteng24ORCID,Wang Yuanming12ORCID,Bœhm Céline4,Djorgovski S G8,Galluccio Laurent9,Delchambre Ludovic3,Connor Thomas710,den Brok Jakob Sebastiaan10ORCID,Do Vale Cunha Pedro H11,Ducourant Christine12,Graham Matthew J8ORCID,Jalan Priyanka13,Klioner Sergei A14,Klüter Jonas15,Mignard François9,Negi Vibhore16ORCID,Petit Quentin12,Scarano Sergio17,Slezak Eric9,Surdej Jean3,Teixeira Ramachrisna11,Walton Dominic J18,Wambsganss Joachim19

Affiliation:

1. Centre for Astrophysics and Supercomputing, Swinburne University of Technology , Hawthorn, Victoria, 3122 , Australia

2. ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav) , Hawthorn, Victoria, 3122 , Australia

3. Space Sciences, Technologies and Astrophysics Research (STAR) Institute, University of Liège , Liege, 4000 , Belgium

4. Sydney Institute for Astronomy, School of Physics, The University of Sydney , Camperdown, NSW 2006 , Australia

5. Donald Bren School of Information and Computer Sciences, University of California , Irvine, CA 92697 , USA

6. CENTRA/SIM , Faculdade de Ciˆencias, Universidade de Lisboa, Ed. C8, Campo Grande, P-1749-016 Lisboa , Portugal

7. Jet Propulsion Laboratory, California Institute of Technology , 4800 Oak Grove Drive, Pasadena, CA 91109 , USA

8. Division of Physics, Mathematics, and Astronomy , Caltech, Pasadena, CA 91125 , USA

9. Université Côte d’Azur , Observatoire de la Côte d’Azur, CNRS, Laboratoire Lagrange, Bd de l’Observatoire, CS 34229, F-06304 Nice cedex 4 , France

10. Center for Astrophysics∣Harvard & Smithsonian , 60 Garden St, 02138 Cambridge, MA , USA

11. Instituto de Astronomia , Geofísica e Ciências Atmosféricas, Universidade de São Paulo, Rua do Matão, 1226, Cidade Universitária, 05508-900 São Paulo, SP , Brazil

12. Laboratoire d’Astrophysique de Bordeaux , Univ. Bordeaux, CNRS, B18N, Allée Geoffroy Saint-Hilaire, F-33615 Pessac , France

13. Center for Theoretical Physics, Polish Academy of Sciences , Warsaw 01-224 , Poland

14. Lohrmann-Observatorium, Technische Universität Dresden , D-01062 Dresden , Germany

15. Department of Physics and Astronomy, Louisiana State University , Baton Rouge, LA 70803 , USA

16. Aryabhatta Research Institute of Observational Sciences (ARIES) , Manora Peak, Nainital 263002 , India

17. Departamento de Física – CCET , Universidade Federal de Sergipe, Rod. Marechal Rondon s/n, 49.100-000, Jardim Rosa Elze, São Cristóvão, SE , Brazil

18. Centre for Astrophysics Research, University of Hertfordshire , College Lane, Hatfield, AL10 9AB , UK

19. Astronomisches Rechen-Institut (ARI) , Zentrum für Astronomie der Universität Heidelberg (ZAH), Mönchhofstr. 12-14, D-69120 Heidelberg , Germany

Abstract

ABSTRACT We present radio observations of 24 confirmed and candidate strongly lensed quasars identified by the Gaia Gravitational Lenses working group. We detect radio emission from eight systems in 5.5 and 9 GHz observations with the Australia Telescope Compact Array (ATCA), and 12 systems in 6 GHz observations with the Karl G. Jansky Very Large Array (VLA). The resolution of our ATCA observations is insufficient to resolve the radio emission into multiple lensed images, but we do detect multiple images from 11 VLA targets. We have analysed these systems using our observations in conjunction with existing optical measurements, including measuring offsets between the radio and optical positions for each image and building updated lens models. These observations significantly expand the existing sample of lensed radio quasars, suggest that most lensed systems are detectable at radio wavelengths with targeted observations, and demonstrate the feasibility of population studies with high-resolution radio imaging.

Funder

Australian Research Council

Fonds De La Recherche Scientifique - FNRS

National Aeronautics and Space Administration

Publisher

Oxford University Press (OUP)

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