4.7 Article

Quasar lenses in the south: searches over the DES public footprint

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 489, Issue 2, Pages 2525-2535

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stz2200

Keywords

catalogues; galaxies: formation; dark matter

Funding

  1. European Union [664931]
  2. VILLUM FONDEN [16599]
  3. Danish council for independent research under the project 'Fundamentals of Dark Matter Structures' [DFF-6108-00470]
  4. CDS, Strasbourg
  5. National Aeronautics and Space Administration - National Science Foundation
  6. U.S. Department of Energy
  7. U.S. National Science Foundation
  8. Ministry of Science and Education of Spain
  9. Science and Technology Facilities Council of the United Kingdom
  10. Higher Education Funding Council for England
  11. NationalCenter for Supercomputing Applications at the University of Illinois at Urbana-Champaign
  12. Center for Cosmology and Astro-Particle Physics at the Ohio State University
  13. Mitchell Institute for Fundamental Physics and Astronomy at Texas AM University
  14. Financiadora de Estudos e Projetos
  15. Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro
  16. Conselho Nacional de Desenvolvimento Cientifico e Tecnologico
  17. Ministerio da Ciencia, Tecnologia e Inovacao
  18. Deutsche Forschungsgemeinschaft
  19. National Science Foundation

Ask authors/readers for more resources

We have scanned 5000 deg(2) of Southern Sky to search for strongly lensed quasars with five methods, all source oriented, but based on different assumptions and selection criteria. We present a list of high-grade candidates from each method (totalling 98 unique, new candidates), to facilitate follow-up spectroscopic campaigns, including two previously unknown quadruplets, WG 210014.9-445206.4 and WG 021416.37-210535.3. We analyse morphological searches based on Gaia multiplet detection and astrometric offsets, fibre-spectroscopic preselection, and X-ray and radio pre-selection. The performance and complementarity of the methods are evaluated on a common sample of known lenses in the Dark Energy Survey public Data Release 1 (DR1) footprint. We recovered in total 13 known lenses, of which 8 are quadruplets. Morphological and colour selection of objects, from the WISE and Gaia-DR2 surveys, recovers most of those known lenses, but searches in the radio and X-ray cover regimes that are beyond the completeness of Gaia. Given the footprint, pre-selection, and depth limits, the current number of quads indicates that the union of these searches is complete, and the expected purity on high-grade candidates is approximate to 60 per cent. Ongoing, spectroscopic campaigns confirm this estimate.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.7
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available