A measurement of the rate of Type Ia supernovae at redshift z ≈ 0.1 from the first season of the SDSS-II Supernova Survey

被引：98

作者：

Dilday, Benjamin ^{[1
,2
]}

Kessler, Richard ^{[2
,3
]}

Frieman, Joshua A. ^{[2
,4
,5
]}

Holtzman, Jon ^{[6
]}

Marriner, John ^{[5
]}

Miknaitis, Gajus ^{[5
]}

Nichol, Robert C. ^{[7
]}

Romani, Roger ^{[8
]}

Sako, Masao ^{[8
,9
]}

Bassett, Bruce ^{[10
,11
]}

Becker, Andrew ^{[12
]}

Cinabro, David ^{[13
]}

DeJongh, Fritz ^{[5
]}

Depoy, Darren L. ^{[14
]}

Doi, Mamoru ^{[15
]}

Garnavich, Peter M. ^{[16
]}

Hogan, Craig J. ^{[12
]}

Jha, Saurabh ^{[8
,17
]}

Konishi, Kohki ^{[18
]}

Lampeitl, Hubert ^{[7
,19
]}

Marshall, Jennifer L. ^{[14
]}

McGinnis, David ^{[5
]}

Prieto, Jose Luis ^{[14
]}

Riess, Adam G. ^{[19
,20
]}

Richmond, Michael W. ^{[21
]}

Schneider, Donald P. ^{[22
]}

Smith, Mathew ^{[7
]}

Takanashi, Naohiro ^{[15
]}

Tokita, Kouichi ^{[15
]}

van der Heyden, Kurt ^{[11
,23
]}

Yasuda, Naoki ^{[18
]}

Zheng, Chen ^{[8
]}

Barentine, John ^{[24
,25
]}

Brewington, Howard ^{[25
]}

Choi, Changsu ^{[26
]}

Crotts, Arlin ^{[27
]}

Dembicky, Jack ^{[25
]}

Harvanek, Michael ^{[25
,28
]}

Im, Myunshin ^{[26
]}

Ketzeback, William ^{[25
]}

Kleinman, Scott J. ^{[25
,29
]}

Krzesinski, Jurek ^{[25
,30
]}

Long, Daniel C. ^{[25
]}

Malanushenko, Elena ^{[25
]}

Malanushenko, Viktor ^{[25
]}

McMillan, Russet J. ^{[25
]}

Nitta, Atsuko ^{[25
,31
]}

Pan, Kaike ^{[25
]}

Saurage, Gabrelle ^{[25
]}

Snedden, Stephanie A. ^{[25
]}

机构：

[1] Univ Chicago, Dept Phys, Chicago, IL 60637 USA

[2] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA

[3] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA

[4] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA

[5] Fermilab Natl Accelerator Lab, Ctr Particle Astrophys, Batavia, IL 60510 USA

[6] New Mexico State Univ, Dept Astron, Las Cruces, NM 88003 USA

[7] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 2EG, Hants, England

[8] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94305 USA

[9] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA

[10] Univ Cape Town, Dept Math & Appl Math, ZA-7701 Rondebosch, South Africa

[11] S African Astron Observ, ZA-7935 Cape Town, South Africa

[12] Univ Washington, Dept Astron, Seattle, WA 98195 USA

[13] Wayne State Univ, Dept Phys, Detroit, MI 48202 USA

[14] Ohio State Univ, Dept Astron, Columbus, OH 43210 USA

[15] Univ Tokyo, Inst Astron, Grad Sch Sci, Tokyo 1810015, Japan

[16] Univ Notre Dame, Notre Dame, IN 46556 USA

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

[18] Univ Tokyo, Inst Cosm Ray Res, Chiba 2778582, Japan

[19] Space Telescope Sci Inst, Baltimore, MD 21218 USA

[20] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA

[21] Rochester Inst Technol, Dept Phys, Rochester, NY 14623 USA

[22] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA

[23] Univ Cape Town, Dept Astron, ZA-7700 Rondebosch, South Africa

[24] Univ Texas Austin, McDonald Observ, Dept Astron, Austin, TX 78712 USA

[25] Apache Point Observ, Sunspot, NM 88349 USA

[26] Seoul Natl Univ, Dept Astron, Seoul, South Korea

[27] Columbia Univ, Dept Astron, New York, NY 10027 USA

[28] Lowell Observ, Flagstaff, AZ 86001 USA

[29] Natl Inst Nat Sci, Natl Astron Observ Japan, Subaru Telescope, Hilo, HI 96720 USA

[30] Akad Pedagogicazna Krakowie, Obserwatorium Astron Suhorze, PL-30084 Krakow, Poland

[31] Gemini Observ, Hilo, HI 96720 USA

来源：

ASTROPHYSICAL JOURNAL | 2008年 / 682卷 / 01期

基金：

英国科学技术设施理事会;

关键词：

supernovae; general;

D O I：

10.1086/587733

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a measurement of the rate of Type Ia supernovae (SNe Ia) from the first of three seasons of data from the SDSS-II Supernova Survey. For this measurement, we include 17 SNe Ia at redshift z ≤ 0.12. Assuming a flat cosmology with Ωm = 0.3 = 1 - ΩΛ, we find a volumetric SN Ia rate of [2:93-0.040 +0.17(systematic)-0.71+0.90(statistical) × 10-5 SNe Mpc-3 h703 yr -1, at a volume-weighted mean redshift of 0.09. This result is consistent with previous measurements of the SN Ia rate in a similar redshift range. The systematic errors are well controlled, resulting in the most precise measurement of the SN Ia rate in this redshift range. We use a maximum likelihood method to fit SN rate models to the SDSS-II Supernova Survey data in combination with other rate measurements, thereby constraining models for the redshift evolution of the SN Ia rate. Fitting the combined data to a simple power-law evolution of the volumetric SN Ia rate, rV ∝ (1 + z)β, we obtain a value of β = 1.5 ± 0.6, i.e., the SN Ia rate is determined to be an increasing function of redshift at the ∼-2.5 σ level. Fitting the results to a model in which the volumetric SN rate is rV = Aρ(t) + Bρ(t), where ρ(t) is the stellar mass density and ρ(t) is the star formation rate, we find A = (2.8 ± 1.2) × 10-14 SNe M⊙-1 yr -1, B = (9.3-3.1+3.4 × 10-4 SNe Mȯ-1. ©2008. The American Astronomical Society. All rights reserved.

引用

页码：262 / 282

页数：21

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