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Optical Observations of the Young Type Ic Supernova SN 2014L in M99
Zhang JJ(张居甲)1,2,3,4; Wang, Xiaofeng5; Vinko, Jozsef6,7,8; Wheeler, J. Craig6; Chang L(常亮)1,3,4; Yang, Yi2,9,12; Wang, Lifan2; Zhai Q(翟倩)1,3,4; Rui, Liming5; Mo, Jun5; Zhang, Tianmeng10; Zhang, Yu11; Wang JG(王建国)1,3,4; Mao JR(毛基荣)1,3,4; Wang CJ(王传军)1,3,4; Yi WM(易卫敏)1,3,4; Xin YX(辛玉新)1,3,4; Li, Wenxiong5; Lun BL(伦宝利)1,3,4; Lu KX(卢开兴)1,3,4; Sai, Hanna5; Zheng XM(郑向明)1,3,4; Zhang XL(张西亮)1,3,4; Zhou, Xu10; Bai JM(白金明)1,3,4
Source PublicationASTROPHYSICAL JOURNAL
2018-08-10
Volume863Issue:1Pages:14
DOI10.3847/1538-4357/aaceaf
Contribution Rank第1完成单位
Indexed BySCI
KeywordSupernovae: Individual (Sn 2014l)
Abstract

We present optical spectroscopic and photometric observations of the nearby type Ic supernova (SN Ic) SN 2014L. This SN was discovered by the Tsinghua-NAOC Transient Survey (TNTS) in the nearby type-Sc spiral galaxy M99((NGC 4254). Fitting to the early-time light curve indicates that SN 2014L was detected at only a few hours after the shock breakout, and it reached a peak brightness of M-V = -17.73 +/- 0.28 mag (L = [2.06 +/- 0.50] x 10(42) erg s(-1)) approximately 13 days later. SN 2014L shows a close resemblance to SN 2007gr in the photometric evolution, while it shows stronger absorption features of intermediate-mass elements (especially Ca II) in the early-time spectra. Based on simple modeling of the observed light curves, we derived the mass of synthesized Ni-56 as M-Ni = 0.075 +/- 0.025 M-circle dot, and the mass and total energy of the ejecta as M-ej = 1.00 +/- 0.20 M-circle dot and E-ej = 1.45 +/- 0.25 foe, respectively. Given these typical explosion parameters, the early detection, and the extensive observations, we suggest that SN 2014L could be a template sample for the investigation of SNe Ic.

Funding ProjectChinese Academy of Sciences (CAS) ; People's Government of Yunnan Province ; National Natural Science Foundation of China (NSFC)[11403096] ; National Natural Science Foundation of China (NSFC)[11773067] ; Major State Basic Research Development Program[2013CB834903] ; National Research, Development and Innovation Office (NKFIH) Hungary - European Union[GINOP-2.3.2-15-2016-00033] ; NSFC[11178003] ; NSFC[11325313] ; NSFC[11633002] ; NSFC[11661161016] ; NSFC[11303085] ; NSFC[11573067] ; Benoziyo Prize Postdoctoral Fellowship ; Western Light Youth Project ; Youth Innovation Promotion Association of the CAS[2018081] ; Youth Innovation Promotion Association of the CAS[2015043] ; Youth Innovation Promotion Association of the CAS[2018080] ; Youth Innovation Promotion Association of the CAS[2016054] ; Key Laboratory for Research in Galaxies and Cosmology of the CAS ; Open Project Program of the Key Laboratory of Optical Astronomy, NAOC, CAS
Funding OrganizationChinese Academy of Sciences (CAS) ; People's Government of Yunnan Province ; National Natural Science Foundation of China (NSFC)[11403096, 11773067] ; Major State Basic Research Development Program[2013CB834903] ; National Research, Development and Innovation Office (NKFIH) Hungary - European Union[GINOP-2.3.2-15-2016-00033] ; NSFC[11178003, 11325313, 11633002, 11661161016, 11303085, 11573067] ; Benoziyo Prize Postdoctoral Fellowship ; Western Light Youth Project ; Youth Innovation Promotion Association of the CAS[2018081, 2015043, 2018080, 2016054] ; Key Laboratory for Research in Galaxies and Cosmology of the CAS ; Open Project Program of the Key Laboratory of Optical Astronomy, NAOC, CAS
Language英语
Subject Area天文学
MOST Discipline Catalogue理学 ; 理学::天文学
SubtypeArticle
PublisherIOP PUBLISHING LTD
Publication PlaceTEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN0004-637X
URL查看原文
WOS IDWOS:000441711100018
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordGamma-ray Burst ; Helium Star Models ; 25 April 1998 ; Light Curves ; Transient 080109 ; Ib Supernovae ; Faint Type ; M51 ; Explosion ; Evolution
Citation statistics
Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/17874
Collection丽江天文观测站(南方基地)
中国科学院天体结构与演化重点实验室
Corresponding AuthorZhang JJ(张居甲)
Affiliation1.Yunnan Observatories (YNAO), Chinese Academy of Sciences, Kunming 650216, People's Republic of China
2.George P. and Cynthia Woods Mitchell Institute for Fundamental Physics & Astronomy, Texas A. & M. University, College Station, TX 77843, USA
3.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650216, People's Republic of China
4.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing, 100012, People's Republic of China
5.Physics Department and Tsinghua Center for Astrophysics (THCA), Tsinghua University, Beijing 100084, People's Republic of China
6.Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Konkoly Thege ut 15-17, Budapest, 1121, Hungary
7.Department of Optics and Quantum Electronics, University of Szeged, H-6720 Szeged, Dómtér 9., Hungary
8.Department of Astronomy, University of Texas at Austin, Austin, TX 78712-1205, USA
9.Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot 76100, Israel
10.National Astronomical Observatories of China (NAOC), Chinese Academy of Sciences, Beijing 100012, People's Republic of China
11.Xinjiang Astronomical Observatory(XAO), Chinese Academy of Sciences, Urumqi, 830011, People's Republic of China
12.Benoziyo Fellow. ORCID iDs
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Corresponding Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Zhang JJ,Wang, Xiaofeng,Vinko, Jozsef,et al. Optical Observations of the Young Type Ic Supernova SN 2014L in M99[J]. ASTROPHYSICAL JOURNAL,2018,863(1):14.
APA Zhang JJ.,Wang, Xiaofeng.,Vinko, Jozsef.,Wheeler, J. Craig.,Chang L.,...&Bai JM.(2018).Optical Observations of the Young Type Ic Supernova SN 2014L in M99.ASTROPHYSICAL JOURNAL,863(1),14.
MLA Zhang JJ,et al."Optical Observations of the Young Type Ic Supernova SN 2014L in M99".ASTROPHYSICAL JOURNAL 863.1(2018):14.
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