THe HST Cluster Supernova Survey. V. Virtual Observatory Resource

Authors
  1. Suzuki N.
  2. Rubin D.
  3. Lidman C.
  4. Aldering G.
  5. Amanullah R.
  6. Barbary K.,Barrientos L.F.
  7. Botyanszki J.
  8. Brodwin M.
  9. Connolly N.
  10. Dawson K.S.,Dey A.
  11. Doi M.
  12. Donahue M.
  13. Deustua S.
  14. Eisenhardt P.
  15. Ellingson E.,Faccioli L.
  16. Fadeyev V.
  17. Fakhouri H.K.
  18. Fruchter A.S.
  19. Gilbank D.G.,Gladders M.D.
  20. Goldhaber G.
  21. Gonzalez A.H.
  22. Goobar A.
  23. Gude A.
  24. Hattori T.,Hoekstra H.
  25. Hsiao E.
  26. Huang X.
  27. Ihara Y.
  28. Jee M.J.
  29. Johnston D.,Kashikawa N.
  30. Koester B.
  31. Konishi K.
  32. Kowalski M.
  33. Linder E.V.
  34. Lubin L.,Melbourne J.
  35. Meyers J.
  36. Morokuma T.
  37. Munshi F.
  38. Mullis C.
  39. Oda T.,Panagia N.
  40. Perlmutter S.
  41. Postman M.
  42. Pritchard T.
  43. Rhodes J.
  44. Ripoche P.,Rosati P.
  45. Schlegel D.J.
  46. Spadafora A.
  47. Stanford S.A.
  48. Stanishev V.,Stern D.
  49. Strovink M.
  50. Takanashi N.
  51. Tokita K.
  52. Wagner M.
  53. Wang L.,Yasuda N.
  54. Yee H.K.C.
  55. Project T.S.C.
  56. Published by
    CDS
Abstract

We present Advanced Camera for Surveys, NICMOS, and Keck adaptive-optics-assisted photometry of 20 Type Ia supernovae (SNe Ia) from the Hubble Space Telescope (HST) Cluster Supernova Survey. The SNe Ia were discovered over the redshift interval 0.623<z<1.415. Of these SNe Ia, 14 pass our strict selection cuts and are used in combination with the world's sample of SNe Ia to derive the best current constraints on dark energy. Of our new SNe Ia, 10 are beyond redshift z = 1, thereby nearly doubling the statistical weight of HST-discovered SNe Ia beyond this redshift. Our detailed analysis corrects for the recently identified correlation between SN Ia luminosity and host galaxy mass and corrects the NICMOS zero point at the count rates appropriate for very distant SNe Ia. Adding these SNe improves the best combined constraint on dark-energy density, {rho}_DE_(z), at redshifts 1.0<z<1.6 by 18% (including systematic errors).

Keywords
  1. hst-photometry
  2. supernovae
  3. redshifted
  4. infrared-sources
Bibliographic source Bibcode
2012ApJ...746...85S
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/746/85
IVOA Identifier IVOID
ivo://CDS.VizieR/J/ApJ/746/85
Document Object Identifer DOI
doi:10.26093/cds/vizier.17460085

Access

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https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/746/85
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/746/85
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/746/85
IVOA Table Access TAP
https://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).
https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/746/85/table1?
https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/746/85/table1?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/746/85/table1?

History

2013-09-26T10:05:02Z
Resource record created
2013-09-26T10:05:02Z
Created
2018-01-04T08:22:26Z
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