| Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the Kepler 2 Observations | |
Li, W.1,2; Wang, X.1; Vinko, J.3,4,5; Mo, J.1; Hosseinzadeh, G.2,6,7; Sand, D. J.8; Zhang JJ(张居甲)9,10,11 ; Lin, H.1; Zhang, T.12; Wang, L.13,14; Zhang, J.1; Chen, Z.1; Xiang, D.1; Rui, L.1; Huang, F.1,15; Li, X.1; Zhang, X.1; Li, L.1; Baron, E.16; Derkacy, J. M.16; Zhao, X.17; Sai, H.1; Zhang, K.1,5; Wang, L.12,18; Howell, D. A.2,6; McCully, C.2; Arcavi, I.2,6,19,77; Valenti, S.20; Hiramatsu, D.2,6; Burke, J.2,6; Rest, A.21,22; Garnavich, P.23; Tucker, B. E.24,25,26; Narayan, G.21,78; Shaya, E.27; Margheim, S.28; Zenteno, A.29; Villar, A.7; Dimitriadis, G.30; Foley, R. J.30; Pan, Y. -C.30; Coulter, D. A.30; Fox, O. D.21; Jha, S. W.31; Jones, D. O.30; Kasen, D. N.32,33; Kilpatrick, C. D.30; Piro, A. L.34; Riess, A. G.21,22; Rojas-Bravo, C.30; Shappee, B. J.35; Holoien, T. W. -S.34,79; Stanek, K. Z.36,37; Drout, M. R.34,80,81; Auchettl, K.36,38; Kochanek, C. S.36,37; Brown, J. S.37; Bose, S.39; Bersier, D.40; Brimacombe, J.41; Chen, P.39; Dong, S.39; Holmbo, S.42; Munoz, J. A.43,44; Mutel, R. L.45; Post, R. S.46; Prieto, J. L.47,48; Shields, J.37; Tallon, D.45; Thompson, T. A.36,37; Vallely, P. J.37; Villanueva, S., Jr.37; Smartt, S. J.49; Smith, K. W.50; Chambers, K. C.51; Flewelling, H. A.51; Huber, M. E.51; Magnier, E. A.51; Waters, C. Z.51; Schultz, A. S. B.51,52; Bulger, J.51; Lowe, T. B.51; Willman, M.51; Sarneczky, K.3; Pal, A.3; Wheeler, J. C.14,53; Bodi, A.3; Bognar, Zs.3; Csak, B.3; Cseh, B.3; Csornyei, G.3; Hanyecz, O.3; Ignacz, B.3; Kalup, Cs.3; Konyves-Toth, R.3; Kriskovics, L.3; Ordasi, A.3; Rajmon, I.54; Sodor, A.3; Szabo, R.3,52; Szakats, R.3; Zsidi, G.3; Milne, P.8; Andrews, J. E.8; Smith, N.8; Bilinski, C.8; Brown, P. J.14,55; Nordin, J.56; Williams, S. C.57; Galbany, L.58; Palmerio, J.59; Hook, I. M.57; Inserra, C.60; Maguire, K.61; Cartier, Regis62; Razza, A.63,64; Gutierrez, C. P.65; Hermes, J. J.66,80; Reding, J. S.66; Kaiser, B. C.66; Tonry, J. L.35; Heinze, A. N.35; Denneau, L.35; Weiland, H.35; Stalder, B.67; Barentsen, G.68,69; Dotson, J.68; Barclay, T.70,71; Gully-Santiago, M.68,69; Hedges, C.68,69; Cody, A. M.68,69; Howell, S.72; Coughlin, J.72,73; Van Cleve, J. E.72,73; Vinicius de Miranda Cardoso, J.72,74; Larson, K. A.75; McCalmont-Everton, K. M.75; Peterson, C. A.75; Ross, S. E.75; Reedy, L. H.76; Osborne, D.76; McGinn, C.76; Kohnert, L.76; Migliorini, L.76; Wheaton, A.76; Spencer, B.76; Labonde, C.76; Castillo, G.76; Beerman, G.76; Steward, K.76; Hanley, M.76; Larsen, R.76; Gangopadhyay, R.76; Kloetzel, R.76; Weschler, T.76; Nystrom, V.76; Moffatt, J.76; Redick, M.76; Griest, K.76; Packard, M.76; Muszynski, M.76; Kampmeier, J.76; Bjella, R.76; Flynn, S.76; Elsaesser, B.76
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| 发表期刊 | ASTROPHYSICAL JOURNAL
 |
| 2019 | |
| 卷号 | 870期号:1页码:33 |
| DOI | 10.3847/1538-4357/aaec74 |
| 产权排序 | 第9完成单位 |
| 收录类别 | SCI |
| 关键词 | supernovae: general supernovae: individual (SN 2018oh) |
| 摘要 | Supernova (SN) 2018oh (ASASSN-18bt) is the first spectroscopically confirmed Type Ia supernova (SN Ia) observed in the Kepler field. The Kepler data revealed an excess emission in its early light curve, allowing us to place interesting constraints on its progenitor system. Here we present extensive optical, ultraviolet, and nearinfrared photometry, as well as dense sampling of optical spectra, for this object. SN 2018oh is relatively normal in its photometric evolution, with a rise time of 18.3 +/- 0.3 days and Delta m(15)(B) = 0.96 +/- 0.03 mag, but it seems to have bluer B - V colors. We construct the "UVOIR" bolometric light curve having a peak luminosity of 1.49. x. 10(43) erg s(-1), from which we derive a nickel mass as 0.55 +/- 0.04M(circle dot) by fitting radiation diffusion models powered by centrally located Ni-56. Note that the moment when nickel-powered luminosity starts to emerge is + 3.85 days after the first light in the Kepler data, suggesting other origins of the early-time emission, e. g., mixing of Ni-56 to outer layers of the ejecta or interaction between the ejecta and nearby circumstellar material or a nondegenerate companion star. The spectral evolution of SN 2018oh is similar to that of a normal SN Ia but is characterized by prominent and persistent carbon absorption features. The C. II features can be detected from the early phases to about 3 weeks after the maximum light, representing the latest detection of carbon ever recorded in an SN Ia. This indicates that a considerable amount of unburned carbon exists in the ejecta of SN 2018oh and may mix into deeper layers. |
| 资助项目 | Ma Huateng Foundation ; Chinese Academy of Sciences ; People's Government of Yunnan Province ; National Natural Science Foundation of China (NSFC)[11325313] ; National Natural Science Foundation of China (NSFC)[11633002] ; National Natural Science Foundation of China (NSFC)[11761141001] ; National Program on Key Research and Development Project[2016YFA0400803] ; Tsinghua University Initiative Scientific Research Program[20161080144] ; Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences[OP201702] ; NSFC[11403096] ; NSFC[11773067] ; NSFC[11573003] ; Key Research Program of the CAS[KJZD-EW-M06] ; Youth Innovation Promotion Association of the CAS[2018081] ; CAS "Light of West China" Program ; US National Science Foundation[1313484] ; US National Science Foundation[AST-1311862] ; NASA through the Einstein Fellowship Program[PF6-170148] ; NASA's Astrophysics Data Analysis Program[NNX13AF35G] ; NSF[AST-1821967] ; NSF[1821987] ; NSF[1813708] ; NSF[1813466] ; NSF[AST-1515927] ; NSF[AST-0908816] ; NSF[AST-1518052] ; Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)[CE170100013] ; NASA[NNX16AB5G] ; NASA[NNG17PX03C] ; NASA[80NSSC18K0303] ; NASA[NAS5-26555] ; project "Transient Astrophysical Objects" of the National Research, Development and Innovation Office (NKFIH), Hungary - European Union[GINOP 2.3.2-15-2016-00033] ; "Lendulet" Program of the Hungarian Academy of Sciences[LP2012-31] ; "Lendulet" Program of the Hungarian Academy of Sciences[LP2018-7/2018] ; NKFIH[K-115709] ; National Research, Development and Innovation Fund of Hungary under PD_17 funding scheme[PD123910] ; NASA through Hubble Fellowship - Space Telescope Science Institute[HST-HF2-51357.001-A] ; NASA K2 Cycle 4[NNX17AE92G] ; ESO program[199.D-0143] ; STFC through an Ernest Rutherford Fellowship ; EU Horizon 2020 ERC grant[758638] ; EU/FP7-ERC[615929] ; Gordon and Betty Moore Foundation[GBMF5490] ; Mt. Cuba Astronomical Foundation ; Center for Cosmology and AstroParticle Physics at Ohio State University ; Chinese Academy of Sciences South America Center for Astronomy (CASSACA) ; Villum Foundation ; Strategic Priority Research Program-The Emergence of Cosmological Structures of the Chinese Academy of Sciences[11 XDB09000000] ; Special Fund for Astronomy from the Ministry of Finance ; Gordon & Betty Moore Foundation ; Heising-Simons Foundation ; Alfred P. Sloan Foundation ; David and Lucile Packard Foundation ; NASA Science Mission directorate ; NASA K2 cycle 4 grant[NNX17AI64G] ; HST[GO-12577] ; HST[HST AR-12851] ; NASA K2 cycle 5 grant[80NSSC18K0302] ; Chinese Academy of Sciences (CAS) |
| 项目资助者 | Ma Huateng Foundation ; Chinese Academy of Sciences ; People's Government of Yunnan Province ; National Natural Science Foundation of China (NSFC)[11325313, 11633002, 11761141001] ; National Program on Key Research and Development Project[2016YFA0400803] ; Tsinghua University Initiative Scientific Research Program[20161080144] ; Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences[OP201702] ; NSFC[11403096, 11773067, 11573003] ; Key Research Program of the CAS[KJZD-EW-M06] ; Youth Innovation Promotion Association of the CAS[2018081] ; CAS "Light of West China" Program ; US National Science Foundation[1313484, AST-1311862] ; NASA through the Einstein Fellowship Program[PF6-170148] ; NASA's Astrophysics Data Analysis Program[NNX13AF35G] ; NSF[AST-1821967, 1821987, 1813708, 1813466, AST-1515927, AST-0908816, AST-1518052] ; Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)[CE170100013] ; NASA[NNX16AB5G, NNG17PX03C, 80NSSC18K0303, NAS5-26555] ; project "Transient Astrophysical Objects" of the National Research, Development and Innovation Office (NKFIH), Hungary - European Union[GINOP 2.3.2-15-2016-00033] ; "Lendulet" Program of the Hungarian Academy of Sciences[LP2012-31] ; Lendulet Program of the Hungarian Academy of Sciences[LP2018-7/2018] ; NKFIH[K-115709] ; National Research, Development and Innovation Fund of Hungary under PD_17 funding scheme[PD123910] ; NASA through Hubble Fellowship - Space Telescope Science Institute[HST-HF2-51357.001-A] ; NASA K2 Cycle 4[NNX17AE92G] ; ESO program[199.D-0143] ; STFC through an Ernest Rutherford Fellowship ; EU Horizon 2020 ERC grant[758638] ; EU/FP7-ERC[615929] ; Gordon and Betty Moore Foundation[GBMF5490] ; Mt. Cuba Astronomical Foundation ; Center for Cosmology and AstroParticle Physics at Ohio State University ; Chinese Academy of Sciences South America Center for Astronomy (CASSACA) ; Villum Foundation ; Strategic Priority Research Program-The Emergence of Cosmological Structures of the Chinese Academy of Sciences[11 XDB09000000] ; Special Fund for Astronomy from the Ministry of Finance ; Gordon & Betty Moore Foundation ; Heising-Simons Foundation ; Alfred P. Sloan Foundation ; David and Lucile Packard Foundation ; NASA Science Mission directorate ; NASA K2 cycle 4 grant[NNX17AI64G] ; HST[GO-12577, HST AR-12851] ; NASA K2 cycle 5 grant[80NSSC18K0302] ; Chinese Academy of Sciences (CAS) |
| 语种 | 英语 |
| 学科领域 | 天文学 ; 恒星与银河系 |
| 文章类型 | Article |
| 出版者 | IOP PUBLISHING LTD |
| 出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
| ISSN | 0004-637X |
| URL | 查看原文 |
| WOS记录号 | WOS:000454551600001 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | HIGH-VELOCITY FEATURES ; WHITE-DWARF MODELS ; LIGHT CURVES ; CIRCUMSTELLAR MATERIAL ; FACTORY OBSERVATIONS ; IMPROVED DISTANCES ; DATA RELEASE ; SN 2011FE ; SPECTRA ; ULTRAVIOLET |
| 引用统计 | |
| 文献类型 | 期刊论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/18805 |
| 专题 | 南方基地 中国科学院天体结构与演化重点实验室 |
| 通讯作者 | Li, W. |
| 作者单位 | 1.Physics Department and Tsinghua Center for Astrophysics (THCA), Tsinghua University, Beijing, 100084, People's Republic of China 2.Las Cumbres Observatory, 6740 Cortona Dr. Ste. 102, Goleta, CA 93117-5575, USA 3.Konkoly Observatory, MTA CSFK, Konkoly Thege M. ut 15-17, Budapest, 1121, Hungary 4.Department of Optics & Quantum Electronics, University of Szeged, Dom ter 9, Szeged, 6720 Hungary 5.Department of Astronomy, University of Texas at Austin, Austin, TX 78712, USA 6.Department of Physics, University of California, Santa Barbara, CA 93106-9530, USA 7.Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA 8.Steward Observatory, University of Arizona, 933 North Cherry Avenue, Rm. N204, Tucson, AZ 85721-0065, USA 9.Yunnan Observatories (YNAO), Chinese Academy of Sciences, Kunming 650216, People's Republic of China 10.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650216, People's Republic of China 11.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing, 100012, People's Republic of China 12.National Astronomical Observatory of China, Chinese Academy of Sciences, Beijing, 100012, People's Republic of China 13.Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210034, People's Republic of China 14.George P. and Cynthia Woods Mitchell Institute for Fundamental Physics & Astronomy, Texas A&M University, Department of Physics and Astronomy, 4242 TAMU, College Station, TX 77843, USA 15.Department of Astronomy, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, People's Republic of China 16.Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman, OK, USA 17.School of Science, Tianjin University of Technology, Tianjin, 300384, People's Republic of China 18.Chinese Academy of Sciences South America Center for Astronomy, China-Chile Joint Center for Astronomy, Camino El Observatorio 1515, Las Condes, Santiago, Chile 19.The Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv 69978, Israel 20.Department of Physics, University of California, Davis, CA 95616, USA 21.Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA 22.Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218, USA 23.Department of Physics, University of Notre Dame, 225 Nieuwland Science Hall, Notre Dame, IN 46556-5670, USA 24.The Research School of Astronomy and Astrophysics, Mount Stromlo Observatory, Australian National University, Canberra, ACT 2611, Australia 25.National Centre for the Public Awareness of Science, Australian National University, Canberra, ACT 2611, Australia 26.The ARC Centre of Excellence for All-Sky Astrophysics in 3 Dimension (ASTRO 3D), Australia 27.Astronomy Department, University of Maryland, College Park, MD 20742-2421, USA 28.Gemini Observatory, Southern Operations Center, c/o AURA, Casilla 603, La Serena, Chile 29.Cerro Tololo Inter-American Observatory, Casilla 603, La Serena, Chile 30.Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064, USA 31.Department of Physics and Astronomy, Rutgers, The State University of New Jersey, 136 Frelinghuysen Road, Piscataway, NJ 08854, USA 32.Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA 33.Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA 34.The Observatories of the Carnegie Institution for Science, 813 Santa Barbara St., Pasadena, CA 91101, USA 35.Institute for Astronomy, University of Hawai'i, 2680 Woodlawn Drive, Honolulu, HI 96822, USA 36.Center for Cosmology and AstroParticle Physics (CCAPP), The Ohio State University, 191 W. Woodruff Ave., Columbus, OH 43210, USA 37.Department of Astronomy, The Ohio State University, 140 West 18th Avenue, Columbus, OH 43210, USA 38.Department of Physics, The Ohio State University, 191 W. Woodruff Avenue, Columbus, OH 43210, USA 39.Kavli Institute for Astronomy and Astrophysics, Peking University, Yi He Yuan Road 5, Hai Dian District, Beijing 100871, People's Republic of China 40.Astrophysics Research Institute, Liverpool John Moores University, 146 Brownlow Hill, Liverpool L3 5RF, UK 41.Coral Towers Observatory, Cairns, QLD 4870, Australia 42.Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark 43.Departamento de Astronomía y Astrofísica, Universidad de Valencia, E-46100 Burjassot, Valencia, Spain 44.Observatorio Astronómico, Universidad de Valencia, E-46980 Paterna, Valencia, Spain 45.Department of Physics and Astronomy, University of Iowa, Iowa City, IA 52242, USA 46.Post Observatory, Lexington, MA 02421, USA 47.Núcleo de Astronomía de la Facultad de Ingeniería, Universidad Diego Portales, Av. Ejército 441, Santiago, Chile 48.Millennium Institute of Astrophysics, Santiago, Chile 49.Astrophysics Research Centre, School of Mathematics and Physics, Queen's University Belfast, Northern Ireland, BT7 1NN, UK 50.Queen's University Belfast, Northern Ireland, BT7 1NN, UK 51.Institute for Astronomy, University of Hawaii at Manoa, 2680 Woodlawn Drive, Honolulu, HI 96822, USA 52.MTA CSFK Lendület Near-Field Cosmology Research Group, Budapest, Hungary 53.Department of Astronomy, University of Texas at Austin, Austin, TX 78712, USA 54.Berzsenyi Dániel High School, Kárpát utca 49-53, Budapest, 1133, Hungary 55.Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station, TX 77843, USA 56.Institute of Physics, Humboldt-Universität zu Berlin, Newtonstr. 15, D-12489 Berlin, Germany 57.Physics Department, Lancaster University, Lancaster LA1 4 YB, UK 58.PITT PACC, Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260, USA 59.Sorbonne Universités, UPMC Univ. Paris 6 et CNRS, UMR 7095, Institut dAstrophysique de Paris, 98 bis bd Arago, F-75014 Paris, France 60.Department of Physics and Astronomy, University of Southampton, Southampton, SO17 1BJ, UK 61.Astrophysics Research Centre, School of Mathematics and Physics, Queen's University Belfast, Belfast BT7 1NN, UK 62.Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, Casilla 603, La Serena, Chile 63.European Southern Observatory, Alonso de Córdova 3107, Casilla 19, Santiago, Chile 64.Departamento de Astronomía, Universidad de Chile, Camino El Observatorio 1515, Las Condes, Santiago, Chile 65.University of Southampton, Southampton, SO17 1BJ, UK 66.Department of Physics and Astronomy, University of North Carolina, Chapel Hill, NC 27599, USA 67.LSST, 950 North Cherry Avenue, Tucson, AZ 85719, USA 68.NASA Ames Research Center, Moffett Blvd., Mountain View, CA 94035, USA 69.Bay Area Environmental Research Institute, P.O. Box 25, Moffett Field, CA 94035, USA 70.NASA Goddard Space Flight Center, 8800 Greenbelt Rd., Greenbelt, MD 20771, USA 71.University of Maryland, Baltimore County, 1000 Hilltop Cir., Baltimore, MD 21250, USA 72.NASA Ames Research Center, Moffett Field, CA 94035, USA 73.SETI Institute, 189 Bernardo Avenue, Mountain View, CA 94043, USA 74.Universidade Federal de Campina Grande, Campina Grande, Brazil 75.Ball Aerospace and Technologies Corp., Boulder, CO 80301, USA 76.LASP, University of Colorado at Boulder, Boulder, CO 80303, USA 77.Einstein Fellow. 78.Lasker Fellow. 79.Carnegie Fellow. 80.Hubble Fellow. 81.Dunlap Fellow. |
| 推荐引用方式 GB/T 7714 | Li, W.,Wang, X.,Vinko, J.,et al. Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the Kepler 2 Observations[J]. ASTROPHYSICAL JOURNAL,2019,870(1):33. |
| APA | Li, W..,Wang, X..,Vinko, J..,Mo, J..,Hosseinzadeh, G..,...&Elsaesser, B..(2019).Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the Kepler 2 Observations.ASTROPHYSICAL JOURNAL,870(1),33. |
| MLA | Li, W.,et al."Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the Kepler 2 Observations".ASTROPHYSICAL JOURNAL 870.1(2019):33. |
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