A TYPE Ia SUPERNOVA AT REDSHIFT 1.55 IN HUBBLE SPACE TELESCOPE INFRARED OBSERVATIONS FROM CANDELS
Creators
- Rodney, Steven A.1
- Riess, Adam G.1
- Jones, David O.1
- Dahlen, Tomas2
- Ferguson, Henry C.2
- Casertano, Stefano2
- Grogin, Norman A.2
- Strolger, Louis-Gregory3
- Hjorth, Jens4
- Frederiksen, Teddy F.4
- Weiner, Benjamin J.5
- Mobasher, Bahram6
- Challis, Peter7
- Kirshner, Robert P.7
- Faber, S. M.8
- Filippenko, Alexei V.9
- Garnavich, Peter10
- Hayden, Brian10
- Graur, Or11
- Jha, Saurabh W.12
- and others
- 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/746/1/5Additional 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