MEASUREMENTS OF THE RATE OF TYPE Ia SUPERNOVAE AT REDSHIFT ≲0.3 FROM THE SLOAN DIGITAL SKY SURVEY II SUPERNOVA SURVEY

被引:79
作者
Dilday, Benjamin [1 ,2 ,3 ]
Smith, Mathew [4 ,5 ]
Bassett, Bruce [4 ,6 ]
Becker, Andrew [7 ]
Bender, Ralf [8 ,9 ]
Castander, Francisco [10 ]
Cinabro, David [11 ]
Filippenko, Alexei V. [12 ]
Frieman, Joshua A. [13 ,14 ]
Galbany, Lluis [15 ]
Garnavich, Peter M. [16 ]
Goobar, Ariel [17 ,18 ]
Hopp, Ulrich [8 ,9 ]
Ihara, Yutaka [19 ]
Jha, Saurabh W. [1 ]
Kessler, Richard [3 ,13 ]
Lampeitl, Hubert [5 ]
Marriner, John [14 ]
Miquel, Ramon [15 ,20 ]
Molla, Mercedes [21 ]
Nichol, Robert C. [5 ]
Nordin, Jakob [18 ]
Riess, Adam G. [22 ,23 ]
Sako, Masao [24 ]
Schneider, Donald P. [25 ]
Sollerman, Jesper [17 ,26 ]
Wheeler, J. Craig [27 ]
Ostman, Linda [18 ]
Bizyaev, Dmitry [28 ]
Brewington, Howard [28 ]
Malanushenko, Elena [28 ]
Malanushenko, Viktor [28 ]
Oravetz, Dan [28 ]
Pan, Kaike [28 ]
Simmons, Audrey [28 ]
Snedden, Stephanie [28 ]
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] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 2EG, Hants, England
[6] S African Astron Observ, ZA-7935 Cape Town, South Africa
[7] Univ Washington, Dept Astron, Seattle, WA 98195 USA
[8] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
[9] Univ Sternwarte, D-81679 Munich, Germany
[10] CSIC, IEEC, Inst Ciencies Espai, Barcelona, Spain
[11] Wayne State Univ, Dept Phys & Astron, Detroit, MI 48202 USA
[12] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
[13] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
[14] Fermilab Natl Accelerator Lab, Ctr Astrophys, Batavia, IL 60510 USA
[15] Inst Fis Altes Energies, Barcelona, Spain
[16] Univ Notre Dame, Notre Dame, IN 46556 USA
[17] Stockholm Univ, Dept Astron, Oskar Klein Ctr, SE-10691 Stockholm, Sweden
[18] Stockholm Univ, Dept Phys, Albanova Univ Ctr, S-10691 Stockholm, Sweden
[19] Univ Tokyo, Grad Sch Sci, Inst Astron, Tokyo 1810015, Japan
[20] Inst Catalana Rec & Estudis Avancats, Barcelona, Spain
[21] Ctr Invest Energet Medioambientales & Tecnol, Madrid, Spain
[22] Space Telescope Sci Inst, Baltimore, MD 21218 USA
[23] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
[24] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA
[25] Penn State Univ, Dept Phys & Astron, Davey Lab 525, University Pk, PA 16802 USA
[26] Univ Copenhagen, Niels Bohr Inst, Dark Cosmol Ctr, DK-1168 Copenhagen, Denmark
[27] Univ Texas Austin, Dept Astron, Austin, TX 78712 USA
[28] Apache Point Observ, Sunspot, NM 88349 USA
基金
美国国家科学基金会;
关键词
supernovae:; general; HUBBLE-SPACE-TELESCOPE; ABSOLUTE MAGNITUDE DISTRIBUTIONS; DARK ENERGY; STAR-FORMATION; LIGHT CURVES; CONSTRAINTS; DISCOVERIES; PHOTOMETRY; MONITOR; DIAGRAM;
D O I
10.1088/0004-637X/713/2/1026
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present ameasurement of the volumetric Type Ia supernova (SN Ia) rate based on data from the Sloan Digital Sky Survey II (SDSS-II) Supernova Survey. The adopted sample of supernovae (SNe) includes 516 SNe Ia at redshift z less than or similar to 0.3, of which 270(52%) are spectroscopically identified as SNe Ia. The remaining 246 SNe Ia were identified through their light curves; 113 of these objects have spectroscopic redshifts from spectra of their host galaxy, and 133 have photometric redshifts estimated from the SN light curves. Based on consideration of 87 spectroscopically confirmed non-Ia SNe discovered by the SDSS-II SN Survey, we estimate that 2.04+(1.61%)(-0.95) -0.95% of the photometric SNe Ia may be misidentified. The sample of SNe Ia used in this measurement represents an order of magnitude increase in the statistics for SN Ia rate measurements in the redshift range covered by the SDSS-II Supernova Survey. If we assume an SN Ia rate that is constant at low redshift (z < 0.15), then the SN observations can be used to infer a value of the SN rate of rV = (2.69(-0.30-0.01)(+ 0.34+ 0.21)) x 10(-5) SNe yr(-1) Mpc(-3) (H-0/(70 km s(-1) Mpc(-1)))(3) at a mean redshift of similar to 0.12, based on 79 SNe Ia of which 72 are spectroscopically confirmed. However, the large sample of SNe Ia included in this study allows us to place constraints on the redshift dependence of the SN Ia rate based on the SDSS-II Supernova Survey data alone. Fitting a power-law model of the SN rate evolution, rV (z) = A(p) x((1 + z)/(1 + z(0)))(nu), over the redshift range 0.0 < z < 0.3 with z0 = 0.21, results in A(p) = (3.43+(+0.15)(-.015) SNe yr-1 Mpc-3 (H-0/(70 km s(-1) Mpc(-1)))(3) and nu = 2.04(-0.89)(+0.89).
引用
收藏
页码:1026 / 1036
页数:11
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