Lick Observatory Supernova Search follow-up program: photometry data release of 93 Type Ia supernovae

被引：54

作者：

Stahl, Benjamin E. ^{[1
,2
]}

Zheng, WeiKang ^{[1
]}

de Jaeger, Thomas ^{[1
]}

Filippenko, Alexei V. ^{[1
,3
,4
]}

Bigley, Andrew ^{[1
]}

Blanchard, Kyle ^{[1
]}

Blanchard, Peter K. ^{[4
]}

Brink, Thomas G. ^{[1
]}

Cargill, Samantha K. ^{[1
]}

Casper, Chadwick ^{[1
]}

Channa, Sanyum ^{[1
]}

Choi, Byung Yun ^{[1
]}

Choksi, Nick ^{[1
]}

Chu, Jason ^{[5
]}

Clubb, Kelsey I. ^{[1
]}

Cohen, Daniel P. ^{[6
]}

Ellison, Michael ^{[1
]}

Falcon, Edward ^{[1
]}

Fazeli, Pegah ^{[1
]}

Fuller, Kiera ^{[1
,6
]}

Ganeshalingam, Mohan ^{[7
]}

Gates, Elinor L. ^{[8
]}

Gould, Carolina ^{[1
]}

Halevi, Goni ^{[1
,9
]}

Hayakawa, Kevin T. ^{[8
]}

Hestenes, Julia ^{[1
]}

Jeffers, Benjamin T. ^{[1
]}

Joubert, Niels ^{[10
]}

Kandrashoff, Michael T. ^{[1
]}

Kim, Minkyu ^{[1
]}

Kim, Haejung ^{[1
]}

Kislak, Michelle E. ^{[1
,11
]}

Kleiser, Io ^{[12
]}

Kong, Jason J. ^{[1
]}

de Kouchkovsky, Maxime ^{[1
]}

Krishnan, Daniel ^{[1
]}

Kumar, Sahana ^{[1
,13
]}

Leja, Joel

Leonard, Erin J. ^{[1
,14
]}

Li, Gary Z. ^{[15
]}

Li, Weidong ^{[1
]}

Lu, Philip ^{[2
,6
]}

Mason, Michelle N. ^{[16
]}

Molloy, Jeffrey ^{[1
]}

Pina, Kenia ^{[1
]}

Rex, Jacob ^{[1
]}

Ross, Timothy W. ^{[1
]}

Stegman, Samantha ^{[1
]}

Tang, Kevin ^{[1
]}

Thrasher, Patrick ^{[1
]}

机构：

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

[2] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

[3] Univ Calif Berkeley, Miller Inst Basic Res Sci, Berkeley, CA 94720 USA

[4] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA

[5] Gemini Observ, 670 N Aohoku Pl, Hilo, HI 96720 USA

[6] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA

[7] Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA

[8] Lick Observ, POB 85, Mt Hamilton, CA 95140 USA

[9] Princeton Univ, Dept Astrophys Sci, 4 Ivy Lane, Princeton, NJ 08544 USA

[10] Stanford Univ, Dept Comp Sci, 353 Serra Mall, Stanford, CA 94305 USA

[11] Netflix Inc, 100 Winchester Cir, Los Gatos, CA 95032 USA

[12] NASA, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA

[13] Florida State Univ, Dept Phys, Tallahassee, FL 32306 USA

[14] Univ Calif Los Angeles, Dept Earth & Space Sci, Los Angeles, CA 90025 USA

[15] Univ Calif Los Angeles, Dept Mech & Aerosp Engn, Los Angeles, CA 90025 USA

[16] Univ Wyoming, Dept Phys & Astron, 1000 E Univ,Dept 3905, Laramie, WY 82071 USA

[17] Guangxi Univ, Dept Phys, Nanning 530004, Peoples R China

[18] Univ Oklahoma, Dept Phys & Astron, 440 W Brooks St, Norman, OK 73019 USA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2019年 / 490卷 / 03期

基金：

中国国家自然科学基金; 美国国家科学基金会;

关键词：

supernovae: general; galaxies: distances and redshifts; BVRI LIGHT CURVES; K-CORRECTIONS; STANDARD STARS; DARK ENERGY; SPECTRA; CONSTRAINTS; ULTRAVIOLET; MAGNITUDES; SAMPLE;

D O I：

10.1093/mnras/stz2742

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present BVRI and unfiltered light curves of 93 Type Ia supernovae (SNe Ia) from the Lick Observatory Supernova Search (LOSS) follow-up program conducted between 2005 and 2018. Our sample consists of 78 spectroscopically normal SNe Ia, with the remainder divided between distinct subclasses (3 SN 1991bg-like, 3 SN 1991T-like, 4 SNe Iax, 2 peculiar, and 3 super-Chandrasekhar events), and has a median redshift of 0.0192. The SNe in our sample have a median coverage of 16 photometric epochs at a cadence of 5.4 d, and the median first observed epoch is similar to 4.6 d before maximum B-band light. We describe how the SNe in our sample are discovered, observed, and processed, and we compare the results from our newly developed automated photometry pipeline to those from the previous processing pipeline used by LOSS. After investigating potential biases, we derive a final systematic uncertainty of 0.03 mag in BVRI for our data set. We perform an analysis of our light curves with particular focus on using template fitting tomeasure the parameters that are useful in standardizing SNe Ia as distance indicators. All of the data are available to the community, and we encourage future studies to incorporate our light curves in their analyses.

引用

页码：3882 / 3907

页数：26

共 15 条

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