High-redshift strong lens candidates from DES Virtual Observatory Resource

Authors
  1. Jacobs C.
  2. Collett T.
  3. Glazebrook K.
  4. McCarthy C.
  5. Qin A.K.
  6. Abbott T.M.C.,Abdalla F.B.
  7. Annis J.
  8. Avila S.
  9. Bechtol K.
  10. Bertin E.
  11. Brooks D.,Buckley-Geer E.
  12. Burke D.L.
  13. Carnero Rosell A.
  14. Carrasco Kind M.,Carretero J.
  15. Da Costa L.N.
  16. Davis C.
  17. De Vicente J.
  18. Desai S.
  19. Diehl H.T.,Doel P.
  20. Eifler T.F.
  21. Flaugher B.
  22. Frieman J.
  23. Garcia-Bellido J.,Gaztanaga E.
  24. Gerdes D.W.
  25. Goldstein D.A.
  26. Gruen D.
  27. Gruendl R.A.,Gschwend J.
  28. Gutierrez G.
  29. Hartley W.G.
  30. Hollowood D.L.
  31. Honscheid K.,Hoyle B.
  32. James D.J.
  33. Kuehn K.
  34. Kuropatkin N.
  35. Lahav O.
  36. Li T.S.
  37. Lima M.,Lin H.
  38. Maia M.A.G.
  39. Martini P.
  40. Miller C.J.
  41. Miquel R.
  42. Nord B.,Plazas A.A.
  43. Sanchez E.
  44. Scarpine V.
  45. Schubnell M.
  46. Serrano S.,Sevilla-Noarbe I.
  47. Smith M.
  48. Soares-Santos M.
  49. Sobreira F.
  50. Suchyta E.,Swanson M.E.C.
  51. Tarle G.
  52. Vikram V.
  53. Walker A.R.
  54. Zhang Y.
  55. Zuntz J.,(The DES Collaboration)
  56. Published by
    CDS
Abstract

We search Dark Energy Survey (DES) Year 3 imaging data for galaxy-galaxy strong gravitational lenses using convolutional neural networks. We generate 250000 simulated lenses at redshifts>0.8 from which we create a data set for training the neural networks with realistic seeing, sky and shot noise. Using the simulations as a guide, we build a catalogue of 1.1 million DES sources with 1.8<g-i<5, 0.6<g-r<3, rmag>19, g_mag>20, and imag>18.2. We train two ensembles of neural networks on training sets consisting of simulated lenses, simulated non-lenses, and real sources. We use the neural networks to score images of each of the sources in our catalogue with a value from 0 to 1, and select those with scores greater than a chosen threshold for visual inspection, resulting in a candidate set of 7301 galaxies. During visual inspection, we rate 84 as "probably" or "definitely" lenses. Four of these are previously known lenses or lens candidates. We inspect a further 9428 candidates with a different score threshold, and identify four new candidates. We present 84 new strong lens candidates, selected after a few hours of visual inspection by astronomers. This catalogue contains a comparable number of high-redshift lenses to that predicted by simulations. Based on simulations, we estimate our sample to contain most discoverable lenses in this imaging and at this redshift range.

Keywords
  1. gravitational-lensing
  2. infrared-photometry
  3. visible-astronomy
  4. broad-band-photometry
  5. redshifted
Bibliographic source Bibcode
2019MNRAS.484.5330J
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/484/5330
IVOA Identifier IVOID
ivo://CDS.VizieR/J/MNRAS/484/5330
Document Object Identifer DOI
doi:10.26093/cds/vizier.74845330

Access

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http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/484/5330
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/484/5330
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/484/5330
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http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).
IVOA Cone Search SCS
For use with a cone search client (e.g., TOPCAT).
http://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/484/5330/table4?
https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/484/5330/table4?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/484/5330/table4?

History

2022-06-10T09:17:04Z
Resource record created
2022-06-10T09:17:04Z
Created
2024-08-19T20:16:56Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr