THE SLOAN DIGITAL SKY SURVEY-II: PHOTOMETRY AND SUPERNOVA IA LIGHT CURVES FROM THE 2005 DATA

被引：171

作者：

Holtzman, Jon A. ^{[1
]}

Marriner, John ^{[2
]}

Kessler, Richard ^{[3
,4
]}

Sako, Masao ^{[5
,6
]}

Dilday, Ben ^{[3
,7
]}

Frieman, Joshua A. ^{[2
,3
,8
]}

Schneider, Donald P. ^{[9
]}

Bassett, Bruce ^{[10
,11
]}

Becker, Andrew ^{[12
]}

Cinabro, David ^{[13
]}

DeJongh, Fritz ^{[3
]}

Depoy, Darren L. ^{[14
]}

Doi, Mamoru ^{[15
]}

Garnavich, Peter M. ^{[16
]}

Hogan, Craig J. ^{[12
]}

Jha, Saurabh ^{[5
,17
]}

Konishi, Kohki ^{[18
]}

Lampeitl, Hubert ^{[19
,20
]}

Marshall, Jennifer L. ^{[14
]}

McGinnis, David ^{[3
]}

Miknaitis, Gajus ^{[3
]}

Nichol, Robert C. ^{[20
]}

Prieto, Jose Luis ^{[14
]}

Riess, Adam G. ^{[19
,21
]}

Richmond, Michael W. ^{[22
]}

Romani, Roger ^{[5
]}

Smith, Mathew ^{[20
]}

Takanashi, Naohiro ^{[15
]}

Tokita, Kouichi ^{[15
]}

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

Yasuda, Naoki ^{[18
]}

Zheng, Chen ^{[5
]}

机构：

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

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

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

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

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

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

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

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

[9] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 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, Grad Sch Sci, Inst Astron, 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] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 2EG, Hants, England

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

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

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

来源：

ASTRONOMICAL JOURNAL | 2008年 / 136卷 / 06期

基金：

英国科学技术设施理事会; 美国国家科学基金会; 美国国家航空航天局;

关键词：

supernovae: general; techniques: photometric;

D O I：

10.1088/0004-6256/136/6/2306

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present ugriz light curves for 146 spectroscopically-confirmed or spectroscopically-probable Type Ia supernovae (SNe) from the 2005 season of the Sloan Digital Sky Survey-II Supernova (SN) survey. The light curves have been constructed using a photometric technique that we call scene modeling, which is described in detail here; the major feature is that SN brightnesses are extracted from a stack of images without spatial resampling or convolution of the image data. This procedure produces accurate photometry along with accurate estimates of the statistical uncertainty, and can be used to derive photometry taken with multiple telescopes. We discuss various tests of this technique that demonstrate its capabilities. We also describe the methodology used for the calibration of the photometry, and present calibrated magnitudes and fluxes for all of the spectroscopic SNe Ia from the 2005 season.

引用

页码：2306 / 2320

页数：15

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