Type Ia Supernova Distances at Redshift >1.5 from the Hubble Space Telescope Multi-cycle Treasury Programs: The Early Expansion Rate

被引：122

作者：

Riess, Adam G. ^{[1
,2
]}

Rodney, Steven A. ^{[3
]}

Scolnic, Daniel M.

Shafer, Daniel L. ^{[1
,4
]}

Strolger, Louis-Gregory ^{[2
]}

Ferguson, Henry C. ^{[2
]}

Postman, Marc ^{[2
]}

Graur, Or ^{[5
,6
]}

Maoz, Dan ^{[7
]}

Jha, Saurabh W. ^{[8
]}

Mobasher, Bahram ^{[9
]}

Casertano, Stefano ^{[2
]}

Hayden, Brian ^{[10
,11
]}

Molino, Alberto ^{[12
]}

Hjorth, Jens ^{[13
]}

Garnavich, Peter M. ^{[14
]}

Jones, David O. ^{[1
]}

Kirshner, Robert P. ^{[5
]}

Koekemoer, Anton M. ^{[2
]}

Grogin, Norman A. ^{[2
]}

Brammer, Gabriel ^{[2
]}

Hemmati, Shoubaneh ^{[15
]}

Dickinson, Mark ^{[16
]}

Challis, Peter M. ^{[5
]}

Wolff, Schuyler ^{[1
]}

Clubb, Kelsey I. ^{[17
]}

Filippenko, Alexei V. ^{[17
,18
]}

Nayyeri, Hooshang ^{[19
]}

Vivian, U. ^{[19
]}

Koo, David C. ^{[20
]}

Faber, Sandra M. ^{[20
]}

Kocevski, Dale ^{[21
]}

Bradley, Larry ^{[2
]}

Coe, Dan ^{[2
]}

机构：

[1] Johns Hopkins Univ, Dept Phys & Astron, 3400 North Charles St, Baltimore, MD 21218 USA

[2] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA

[3] Univ South Carolina, Dept Phys & Astron, 712 Main St, Columbia, SC 29208 USA

[4] Univ Chicago, Kavli Inst Cosmol Phys, 5640 South Ellis Ave, Chicago, IL 60637 USA

[5] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA

[6] Amer Museum Nat Hist, Dept Astrophys, Cent Pk West & 79th St, New York, NY 10024 USA

[7] Tel Aviv Univ, Sch Phys & Astron, IL-69978 Tel Aviv, Israel

[8] Rutgers State Univ, Dept Phys & Astron, Piscataway, NJ 08854 USA

[9] Univ Calif Riverside, Dept Phys & Astron, 900 Univ Ave, Riverside, CA 92521 USA

[10] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA

[11] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

[12] Univ Sao Paulo, Inst Astron Geofis & Ciencias Atmosfer, BR-05508090 Sao Paulo, Brazil

[13] Univ Copenhagen, Niels Bohr Inst, Dark Cosmol Ctr, Juliane Maries Vej 30, DK-2100 Copenhagen, Denmark

[14] Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA

[15] CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA

[16] Natl Opt Astron Observ, 950 North Cherry Ave, Tucson, AZ 85719 USA

[17] Univ Calif Berkeley, Dept Astron, 601 Campbell Hall, Berkeley, CA 94720 USA

[18] Univ Calif Berkeley, Miller Inst Basic Res Sci, Berkeley, CA 94720 USA

[19] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA

[20] Univ Calif Santa Cruz, Dept Astron & Astrophys, Santa Cruz, CA 95064 USA

[21] Colby Coll, 4000 Mayflower Hill Dr, Waterville, ME 04901 USA

来源：

ASTROPHYSICAL JOURNAL | 2018年 / 853卷 / 02期

基金：

巴西圣保罗研究基金会;

关键词：

cosmology: observations; methods: observational; supernovae: general; WHITE-DWARF MODELS; DARK ENERGY; SN; 2011FE; UNIVERSE; CONSTRAINTS; HISTORY; ACCELERATION; Z-GREATER-THAN-1; NUCLEOSYNTHESIS; DECELERATION;

D O I：

10.3847/1538-4357/aaa5a9

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present an analysis of 15 Type Ia supernovae (SNe Ia) at redshift z > 1 (9 at 1.5 < z < 2.3) recently discovered in the CANDELS and CLASH Multi-Cycle Treasury programs using WFC3 on the Hubble Space Telescope. We combine these SNe. Ia with a new compilation of similar to 1050 SNe Ia, jointly calibrated and corrected for simulated survey biases to produce accurate distance measurements. We present unbiased constraints on the expansion rate at six redshifts in the range 0.07 < z < 1.5 based only on this combined SN Ia sample. The added leverage of our new sample at z > 1.5 leads to a factor of similar to 3 improvement in the determination of the expansion rate at z = 1.5, reducing its uncertainty to similar to 20%, a measurement of H(z = 1.5)/H-0 = 2.69(-0.52)(+0.86). We then demonstrate that these six derived expansion rate measurements alone provide a nearly identical characterization of dark energy as the full SN sample, making them an efficient compression of the SN Ia data. The new sample of SNe Ia at z > 1.5 usefully distinguishes between alternative cosmological models and unmodeled evolution of the SN Ia distance indicators, placing empirical limits on the latter. Finally, employing a realistic simulation of a potential Wide-Field Infrared Survey Telescope SN survey observing strategy, we forecast optimistic future constraints on the expansion rate from SNe Ia.

引用

页数：15

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Type Ia Supernova Distances at Redshift &gt;1.5 from the Hubble Space Telescope Multi-cycle Treasury Programs: The Early Expansion Rate

Type Ia Supernova Distances at Redshift >1.5 from the Hubble Space Telescope Multi-cycle Treasury Programs: The Early Expansion Rate