A MEASUREMENT OF THE RATE OF TYPE Ia SUPERNOVAE IN GALAXY CLUSTERS FROM THE SDSS-II SUPERNOVA SURVEY

被引：42

作者：

Dilday, Benjamin ^{[1
,2
,3
]}

Bassett, Bruce ^{[4
,5
]}

Becker, Andrew ^{[6
]}

Bender, Ralf ^{[7
,8
]}

Castander, Francisco ^{[9
]}

Cinabro, David ^{[10
]}

Frieman, Joshua A. ^{[11
,12
]}

Galbany, Lluis ^{[13
]}

Garnavich, Peter ^{[14
]}

Goobar, Ariel ^{[15
,16
]}

Hopp, Ulrich ^{[7
,8
]}

Ihara, Yutaka ^{[17
]}

Jha, Saurabh W. ^{[1
]}

Kessler, Richard ^{[3
,11
]}

Lampeitl, Hubert ^{[18
]}

Marriner, John ^{[12
]}

Miquel, Ramon ^{[13
,19
]}

Molla, Mercedes ^{[20
]}

Nichol, Robert C. ^{[18
]}

Nordin, Jakob ^{[16
]}

Riess, Adam G. ^{[21
,22
]}

Sako, Masao ^{[23
]}

Schneider, Donald P. ^{[24
]}

Smith, Mathew ^{[4
,18
]}

Sollerman, Jesper ^{[15
,25
]}

Wheeler, J. Craig ^{[26
]}

Ostman, Linda ^{[16
]}

Bizyaev, Dmitry ^{[27
]}

Brewington, Howard ^{[27
]}

Malanushenko, Elena ^{[27
]}

Malanushenko, Viktor ^{[27
]}

Oravetz, Dan ^{[27
]}

Pan, Kaike ^{[27
]}

Simmons, Audrey ^{[27
]}

Snedden, Stephanie ^{[27
]}

机构：

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

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

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

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

[5] S African Astron Observ, ZA-7935 Observatory, South Africa

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

[7] Max Planck Inst Extraterr Phys, D-85748 Munich, Germany

[8] Univ Sternwarte Munich, D-81679 Munich, Germany

[9] CSIC, IEEC, Inst Ciencies Espai, Barcelona, Spain

[10] Wayne State Univ, Dept Phys & Astron, Detroit, MI 48202 USA

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

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

[13] Inst Fis Altes Energies, Barcelona, Spain

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

[15] Stockholm Univ, Dept Astron, Oskar Klein Ctr, SE-10691 Stockholm, Sweden

[16] Stockholm Univ, Dept Phys, Albanova Univ Ctr, S-10691 Stockholm, Sweden

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

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

[19] Inst Catalana Recerca & Estudis Avancats, Barcelona, Spain

[20] Ctr Invest Energet Medioambientales & Tecnol, Madrid, Spain

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

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

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

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

[25] Univ Copenhagen, Niels Bohr Inst, Dark Cosmol Ctr, DK-1168 Copenhagen, Denmark

[26] Univ Texas Austin, Dept Astron, Austin, TX 78712 USA

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

来源：

ASTROPHYSICAL JOURNAL | 2010年 / 715卷 / 02期

基金：

美国国家科学基金会; 美国国家航空航天局;

关键词：

supernovae:; general; DIGITAL SKY SURVEY; DATA RELEASE; INTERGALACTIC SUPERNOVAE; STAR-FORMATION; LEGACY SURVEY; TELESCOPE; SEARCH; SYSTEM; MAGNITUDES; PHOTOMETRY;

D O I：

10.1088/0004-637X/715/2/1021

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present measurements of the Type Ia supernova (SN) rate in galaxy clusters based on data from the Sloan Digital Sky Survey-II (SDSS-II) Supernova Survey. The cluster SN Ia rate is determined from 9 SN events in a set of 71 C4 clusters at z <= 0.17 and 27 SN events in 492 maxBCG clusters at 0.1 <= z <= 0.3. We find values for the cluster SN Ia rate of (0.37(-0.12-0.01)(+0.17+0.01)) SNur h(2) and (0.55(-0.11-0.01)(+0.13+0.02)) SNur h(2) (SNux = 10(-12) Lx(circle dot)(-1)yr(-1)) in C4 and maxBCG clusters, respectively, where the quoted errors are statistical and systematic, respectively. The SN rate for early-type galaxies is found to be (0.31(-0.12-0.01)(+0.18+0.01)) SNur h(2) and (0.49(-0.11-0.01)(+0.15+0.02)) SNur h(2) in C4 and maxBCG clusters, respectively. The SN rate for the brightest cluster galaxies (BCG) is found to be (2.04(-1.11-0.04)(+1.99+0.07)) SNur h(2) and (0.36(-0.30-0.01)(+0.84+0.01)) SNur h(2) in C4 and maxBCG clusters, respectively. The ratio of the SN Ia rate in cluster early-type galaxies to that of the SN Ia rate in field early-type galaxies is 1.94(-0.91-0.015)(+1.31+0.043) and 3.02(-1.03-0.048)(+1.31+0.062), for C4 and maxBCG clusters, respectively. The SN rate in galaxy clusters as a function of redshift, which probes the late time SN Ia delay distribution, shows only weak dependence on redshift. Combining our current measurements with previous measurements, we fit the cluster SN Ia rate data to a linear function of redshift, and find r(L) =[(0.49(-0.14)(+0.15))+(0.91(-0.81)(+0.85)) x z] SNuB h(2). A comparison of the radial distribution of SNe in cluster to field early-type galaxies shows possible evidence for an enhancement of the SN rate in the cores of cluster early-type galaxies. With an observation of at most three hostless, intra-cluster SNe Ia, we estimate the fraction of cluster SNe that are hostless to be (9.4(-5.1)(+8.3))%.

引用

页码：1021 / 1035

页数：15

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