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

被引:40
|
作者
Rodney, Steven A. [1 ]
Riess, Adam G. [1 ,2 ]
Dahlen, Tomas [2 ]
Strolger, Louis-Gregory [3 ]
Ferguson, Henry C. [2 ]
Hjorth, Jens [4 ]
Frederiksen, Teddy F. [4 ]
Weiner, Benjamin J. [5 ]
Mobasher, Bahram [6 ]
Casertano, Stefano [2 ]
Jones, David O. [1 ]
Challis, Peter [7 ]
Faber, S. M. [8 ]
Filippenko, Alexei V. [9 ]
Garnavich, Peter [10 ]
Graur, Or [11 ]
Grogin, Norman A. [2 ]
Hayden, Brian [10 ]
Jha, Saurabh W. [12 ]
Kirshner, Robert P. [7 ]
Kocevski, Dale [8 ]
Koekemoer, Anton [2 ]
McCully, Curtis [12 ]
Patel, Brandon [12 ]
Rajan, Abhijith [2 ]
Scarlata, Claudia [13 ]
机构
[1] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
[2] Space Telescope Sci Inst, Baltimore, MD 21218 USA
[3] Western Kentucky Univ, Dept Phys, Bowling Green, KY 42101 USA
[4] Univ Copenhagen, Niels Bohr Inst, Dark Cosmol Ctr, DK-2100 Copenhagen, Denmark
[5] Univ Arizona, Dept Astron, Tucson, AZ 85721 USA
[6] Univ Calif Riverside, Dept Phys & Astron, Riverside, CA 92521 USA
[7] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[8] Univ Calif Santa Cruz, Dept Astron & Astrophys, Santa Cruz, CA 92064 USA
[9] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
[10] Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA
[11] Tel Aviv Univ, Dept Astrophys, IL-69978 Tel Aviv, Israel
[12] Rutgers State Univ, Dept Phys & Astron, Piscataway, NJ 08854 USA
[13] Univ Minnesota, Dept Astron, Minneapolis, MN 55455 USA
来源
ASTROPHYSICAL JOURNAL | 2012年 / 746卷 / 01期
基金
新加坡国家研究基金会;
关键词
supernovae:; general; DARK ENERGY; ACCELERATING UNIVERSE; LIGHT CURVES; SNE-IA; CONSTRAINTS; EQUATION; DISCOVERIES; FRACTIONS; SEARCH; RATES;
D O I
10.1088/0004-637X/746/1/5
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 approximate to 2, providing a complementary constraint on SN Ia progenitor models.
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页数:9
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