Published February 10, 2012 | Version v1
Journal article

A TYPE Ia SUPERNOVA AT REDSHIFT 1.55 IN HUBBLE SPACE TELESCOPE INFRARED OBSERVATIONS FROM CANDELS

  • 1. Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218 (United States)
  • 2. Space Telescope Science Institute, Baltimore, MD 21218 (United States)
  • 3. Department of Physics, Western Kentucky University, Bowling Green, KY 42101 (United States)
  • 4. Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen (Denmark)
  • 5. Department of Astronomy, University of Arizona, Tucson, AZ 85721 (United States)
  • 6. Department of Physics and Astronomy, University of California, Riverside, CA 92521 (United States)
  • 7. Harvard/Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States)
  • 8. Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 92064 (United States)
  • 9. Department of Astronomy, University of California, Berkeley, CA 94720-3411 (United States)
  • 10. Department of Physics, University of Notre Dame, Notre Dame, IN 46556 (United States)
  • 11. Department of Astrophysics, Tel Aviv University, 69978 Tel Aviv (Israel)
  • 12. Department of Physics and Astronomy, Rutgers, State University of New Jersey, Piscataway, NJ 08854 (United States)

Description

We report the discovery of a Type Ia supernova (SN Ia) at redshift z = 1.55 with the infrared detector of the Wide Field Camera 3 (WFC3-IR) on the Hubble Space Telescope (HST). This object was discovered in CANDELS imaging data of the Hubble Ultra Deep Field and followed as part of the CANDELS+CLASH Supernova project, comprising the SN search components from those two HST multi-cycle treasury programs. This is the highest redshift SN Ia with direct spectroscopic evidence for classification. It is also the first SN Ia at z > 1 found and followed in the infrared, providing a full light curve in rest-frame optical bands. The classification and redshift are securely defined from a combination of multi-band and multi-epoch photometry of the SN, ground-based spectroscopy of the host galaxy, and WFC3-IR grism spectroscopy of both the SN and host. This object is the first of a projected sample at z > 1.5 that will be discovered by the CANDELS and CLASH programs. The full CANDELS+CLASH SN Ia sample will enable unique tests for evolutionary effects that could arise due to differences in SN Ia progenitor systems as a function of redshift. This high-z sample will also allow measurement of the SN Ia rate out to z ≈ 2, providing a complementary constraint on SN Ia progenitor models.

Availability note (English)

Available from http://dx.doi.org/10.1088/0004-637X/746/1/5

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
746
Journal Issue
1
Journal Page Range
[9 p.]
ISSN
0004-637X
CODEN
ASJOAB

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
43098961
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
CAMERAS; GALAXIES; PHOTOMETRY; RED SHIFT; SPECTROSCOPY; SUPERNOVAE; TELESCOPES
Descriptors DEC
BINARY STARS; ERUPTIVE VARIABLE STARS; STARS; VARIABLE STARS