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.

引用

页数：9

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