The Data Release of the Sloan Digital Sky Survey-II Supernova Survey

被引：118

作者：

Sako, Masao ^{[1
]}

Bassett, Bruce ^{[2
,3
,4
]}

Becker, Andrew C. ^{[5
]}

Brown, Peter J. ^{[6
]}

Campbell, Heather ^{[7
]}

Wolf, Rachel ^{[1
]}

Cinabro, David ^{[8
]}

D'Andrea, Chris B. ^{[1
]}

Dawson, Kyle S. ^{[9
]}

DeJongh, Fritz ^{[10
]}

Depoy, Darren L. ^{[6
]}

Dilday, Ben ^{[11
]}

Doi, Mamoru ^{[12
,13
]}

Filippenko, Alexei V. ^{[14
]}

Fischer, John A. ^{[1
]}

Foley, Ryan J. ^{[15
]}

Frieman, Joshua A. ^{[10
,16
,17
]}

Galbany, Lluis ^{[18
]}

Garnavich, Peter M. ^{[19
]}

Goobar, Ariel ^{[20
,21
]}

Gupta, Ravi R. ^{[22
]}

Hill, Gary J. ^{[23
]}

Hayden, Brian T. ^{[22
]}

Hlozek, Renee ^{[24
,25
]}

Holtzman, Jon A. ^{[26
]}

Hopp, Ulrich ^{[27
,28
]}

Jha, Saurabh W. ^{[29
]}

Kessler, Richard ^{[16
,17
]}

Kollatschny, Wolfram ^{[30
]}

Leloudas, Giorgos ^{[31
]}

Marriner, John ^{[10
]}

Marshall, Jennifer L. ^{[6
]}

Miquel, Ramon ^{[32
,33
]}

Morokuma, Tomoki ^{[12
]}

Mosher, Jennifer ^{[1
]}

Nichol, Robert C. ^{[34
]}

Nordin, Jakob ^{[35
]}

Olmstead, Matthew D. ^{[36
]}

Ostman, Linda ^{[20
,21
]}

Prieto, Jose L. ^{[37
,38
]}

Richmond, Michael ^{[39
]}

Romani, Roger W. ^{[40
]}

Sollerman, Jesper ^{[20
,41
]}

Stritzinger, Max ^{[42
]}

Schneider, Donald P. ^{[43
]}

Smith, Mathew ^{[44
]}

Wheeler, J. Craig ^{[45
]}

Yasuda, Naoki ^{[12
,13
]}

Zheng, Chen ^{[46
]}

机构：

[1] Univ Penn, Dept Phys & Astron, 209 South 33rd St, Philadelphia, PA 19104 USA

[2] African Inst Math Sci, ZA-7945 Cape Town, South Africa

[3] South African Astron Observ, Cape Town, South Africa

[4] Univ Cape Town, Dept Math & Appl Math, Cape Town, South Africa

[5] Univ Washington, Dept Astron, Box 351580, Seattle, WA 98195 USA

[6] Texas A&M Univ, Dept Phys & Astron, College Stn, TX 77843 USA

[7] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England

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

[9] Univ Utah, Dept Phys & Astron, Salt Lake City, UT 84112 USA

[10] Fermilab Natl Accelerator Lab, Ctr Particle Astrophys, POB 500, Batavia, IL 60510 USA

[11] North Idaho Coll, 1000 W Garden Ave, Coeur Dalene, ID 83814 USA

[12] Univ Tokyo, Grad Sch Sci, Inst Astron, 2-21-1 Osawa, Mitaka, Tokyo 1810015, Japan

[13] Univ Tokyo, Todai Inst Adv Study, Kavli Inst Phys & Math Universe Kavli IPMU, WPI, Kashiwa, Chiba 2778583, Japan

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

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

[16] Univ Chicago, Dept Astron & Astrophys, 5640 South Ellis Ave, Chicago, IL 60637 USA

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

[18] Univ Pittsburgh, Dept Phys & Astron, PITT PACC, Pittsburgh, PA 15260 USA

[19] Univ Notre Dame, Dept Phys, 225 Nieuwland Sci Hall, Notre Dame, IN 46556 USA

[20] Stockholm Univ, Oskar Klein Ctr, SE-10691 Stockholm, Sweden

[21] Stockholm Univ, Dept Phys, SE-10691 Stockholm, Sweden

[22] Lawrence Berkeley Natl Lab, 1 Cyclotron Rd MS 50B-4206, Berkeley, CA 94720 USA

[23] Univ Texas Austin, McDonald Observ, Austin, TX 78712 USA

[24] Univ Toronto, Dunlap Inst, Toronto, ON, Canada

[25] Univ Toronto, Dept Astron & Astrophys, Toronto, ON, Canada

[26] New Mexico State Univ, Dept Astron, MSC 4500,POB 30001, Las Cruces, NM 88003 USA

[27] Univ Sternwarte Munich, Scheiner Str 1, D-81679 Munich, Germany

[28] MPI F Extraterr Phys, Giessenbachstr, D-85741 Garching, Germany

[29] Rutgers State Univ, Dept Phys & Astron, 136 Frelinghuysen Rd, Piscataway, NJ 08854 USA

[30] Russian Acad Sci, Special Astrophys Observ, Nizhnii Arkhyz 369167, Karachaevo Cher, Russia

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

[32] Inst Fis Altes Energies, E-08193 Bellaterra, Barcelona, Spain

[33] Inst Catalana Recerca & Estudis Avancats, E-08010 Barcelona, Spain

[34] Univ Portsmouth, Inst Cosmol & Gravitat, Dennis Sciama Bldg,Burnaby Rd, Portsmouth PO1 3FX, Hants, England

[35] Humboldt Univ, Inst Phys, Newtonstr 15, D-12489 Berlin, Germany

[36] Kings Coll, Dept Chem & Phys, 133 North River St, Wilkes Barre, PA 18711 USA

[37] Univ Diego Portales, Nucleo Astron, Fac Ingn, Ave Ejercito 441, Santiago, Chile

[38] Millennium Inst Astrophys, Santiago, Chile

[39] Rochester Inst Technol, Sch Phys & Astron, Rochester, NY 14623 USA

[40] Stanford Univ, Dept Phys, Palo Alto, CA 94305 USA

[41] Stockholm Univ, Dept Astron, SE-10691 Stockholm, Sweden

[42] Aarhus Univ, Dept Phys & Astron, Ny Munkegade 120, DK-8000 Aarhus C, Denmark

[43] Penn State Univ, Dept Astron & Astrophys, 525 Davey Lab, University Pk, PA 16802 USA

[44] Univ Southampton, Dept Phys & Astron, Southampton SO17 1BJ, Hants, England

[45] Univ Texas Austin, Dept Astron, RLM 15308, Austin, TX 78712 USA

[46] 10497 Anson Ave, Cupertino, CA 95014 USA

来源：

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC | 2018年 / 130卷 / 988期

基金：

瑞典研究理事会; 美国国家航空航天局; 美国国家科学基金会;

关键词：

cosmology: observations; supernovae: general; surveys; IA SUPERNOVAE; STAR-FORMATION; LIGHT CURVES; PHOTOMETRIC CLASSIFICATION; HOST GALAXIES; TELESCOPE; CONSTRAINTS; CALIBRATION; RESOLUTION; MASS;

D O I：

10.1088/1538-3873/aab4e0

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

This paper describes the data release of the Sloan Digital Sky Survey-II (SDSS-II) Supernova Survey conducted between 2005 and 2007. Light curves, spectra, classifications, and ancillary data are presented for 10,258 variable and transient sources discovered through repeat ugriz imaging of SDSS Stripe 82, a 300 deg(2) area along the celestial equator. This data release is comprised of all transient sources brighter than r similar or equal to 22.5 mag with no history of variability prior to 2004. Dedicated spectroscopic observations were performed on a subset of 889 transients, as well as spectra for thousands of transient host galaxies using the SDSS-III BOSS spectrographs. Photometric classifications are provided for the candidates with good multi-color light curves that were not observed spectroscopically, using host galaxy redshift information when available. From these observations, 4607 transients are either spectroscopically confirmed, or likely to be, supernovae, making this the largest sample of supernova candidates ever compiled. We present a new method for SN host-galaxy identification and derive host-galaxy properties including stellar masses, star formation rates, and the average stellar population ages from our SDSS multi-band photometry. We derive SALT2 distance moduli for a total of 1364 SN. Ia with spectroscopic redshifts as well as photometric redshifts for a further 624 purely photometric SN. Ia candidates. Using the spectroscopically confirmed subset of the three-year SDSS-II SN. Ia sample and assuming a flat.CDM cosmology, we determine Omega(M) = 0.315 +/- 0.093 (statistical error only) and detect a non-zero cosmological constant at 5.7 sigma.

引用

页数：32

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