SN 2010mb , the SIMBAD biblio

SN 2010mb , the SIMBAD biblio (31 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST02:07:25


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Title First 3 Authors
2012CBET.3309....1B 39 T       O X         3 1 Supernova 2010mb. BEN-AMI S., GAL-YAM A. and QUIMBY R.
2013ApJ...779...98H 42           X         1 12 76 Two superluminous supernovae from the early universe discovered by the supernova legacy survey. HOWELL D.A., KASEN D., LIDMAN C., et al.
2014ApJ...785...37B viz 2502 T   A     X C       62 16 29 SN 2010mb: direct evidence for a supernova interacting with a large amount of hydrogen-free circumstellar material. BEN-AMI S., GAL-YAM A., MAZZALI P.A., et al.
2014ApJ...789...23K viz 16       D               1 344 44 The host galaxies of fast-ejecta core-collapse supernovae. KELLY P.L., FILIPPENKO A.V., MODJAZ M., et al.
2014MNRAS.444.2096N 82           X         2 17 135 Superluminous supernovae from PESSTO. NICHOLL M., SMARTT S.J., JERKSTRAND A., et al.
2015ApJ...799..107W 80             C       1 15 47 Superluminous supernovae powered by magnetars: late-time light curves and hard emission leakage. WANG S.Q., WANG L.J., DAI Z.G., et al.
2015MNRAS.449.1954P 40           X         1 38 19 Massive stars exploding in a He-rich circumstellar medium - VI. Observations of two distant Type Ibn supernova candidates discovered by La Silla-QUEST. PASTORELLO A., HADJIYSKA E., RABINOWITZ D., et al.
2015ApJ...807..147W 80             C       1 9 20 A unified energy-reservoir model containing contributions from 56Ni and neutron stars and its implication for luminous type IC supernovae. WANG S.Q., WANG L.J., DAI Z.G., et al.
2015MNRAS.452.3869N 41           X         1 55 156 On the diversity of superluminous supernovae: ejected mass as the dominant factor. NICHOLL M., SMARTT S.J., JERKSTRAND A., et al.
2016ApJ...829...17S 128           X         3 7 60 Type I superluminous supernovae as explosions inside non-hydrogen circumstellar envelopes. SOROKINA E., BLINNIKOV S., NOMOTO K., et al.
2016ApJ...831..144L 43           X         1 14 54 PS1-14bj: a hydrogen-poor superluminous supernova with a long rise and slow decay. LUNNAN R., CHORNOCK R., BERGER E., et al.
2017ApJ...835...13J 45           X         1 22 99 Long-duration superluminous supernovae at late times. JERKSTRAND A., SMARTT S.J., INSERRA C., et al.
2017ApJ...835...64G 19       D               1 91 351 An open catalog for supernova data. GUILLOCHON J., PARRENT J., KELLEY L.Z., et al.
2016A&A...596A..67R 40           X         1 60 14 SN 2012aa: A transient between Type Ibc core-collapse and superluminous supernovae. ROY R., SOLLERMAN J., SILVERMAN J.M., et al.
2017ApJ...845...85L viz 42           X         1 47 77 Analyzing the largest spectroscopic data set of hydrogen-poor super-luminous supernovae. LIU Y.-Q., MODJAZ M. and BIANCO F.B.
2018ApJ...866L..24N 83           X         2 11 12 One thousand days of SN2015bn: HST imaging shows a light curve flattening consistent with magnetar predictions. NICHOLL M., BLANCHARD P.K., BERGER E., et al.
2018A&A...618A..37F viz 82           X         2 19 10 Oxygen and helium in stripped-envelope supernovae. FREMLING C., SOLLERMAN J., KASLIWAL M.M., et al.
2019A&A...621A..64T 794   K       X C       18 12 6 The luminous late-time emission of the type-Ic supernova iPTF15dtg - evidence for powering from a magnetar? TADDIA F., SOLLERMAN J., FREMLING C., et al.
2019MNRAS.484.3443M 84           X         2 7 1 Synthetic spectra of energetic core-collapse supernovae and the early spectra of SN 2007bi and SN 1999as. MORIYA T.J., MAZZALI P.A. and TANAKA M.
2019ApJ...881...87G viz 419           X C       9 20 27 SN 2016iet: the pulsational or pair instability explosion of a low-metallicity massive CO core embedded in a dense hydrogen-poor circumstellar medium. GOMEZ S., BERGER E., NICHOLL M., et al.
2019MNRAS.489.3591P viz 42           X         1 164 31 Anomaly detection in the Open Supernova Catalog. PRUZHINSKAYA M.V., MALANCHEV K.L., KORNILOV M.V., et al.
2020ApJ...902..139K viz 85           X         2 22 5 Direct evidence of two-component ejecta in Supernova 2016gkg from nebular spectroscopy. KUNCARAYAKTI H., FOLATELLI G., MAEDA K., et al.
2021ApJS..255...29S viz 17       D               1 893 63 The Palomar Transient Factory core-collapse supernova host-galaxy sample. I. Host-galaxy distribution functions and environment dependence of core-collapse supernovae. SCHULZE S., YARON O., SOLLERMAN J., et al.
2022ApJ...928..151F 18       D               1 201 16 Statistical Properties of the Nebular Spectra of 103 Stripped-envelope Core-collapse Supernovae. FANG Q., MAEDA K., KUNCARAYAKTI H., et al.
2022ApJ...939..105B 224       S   X         4 121 10 Seven Years of Coordinated Chandra-NuSTAR Observations of SN 2014C Unfold the Extreme Mass-loss History of Its Stellar Progenitor. BRETHAUER D., MARGUTTI R., MILISAVLJEVIC D., et al.
2022ApJ...941L..32K 90             C       3 16 4 Late-time H/He-poor Circumstellar Interaction in the Type Ic Supernova SN 2021ocs: An Exposed Oxygen-Magnesium Layer and Extreme Stripping of the Progenitor. KUNCARAYAKTI H., MAEDA K., DESSART L., et al.
2023ApJ...950...14R 467           X C       9 38 1 Near-infrared and Optical Observations of Type Ic SN 2021krf: Luminous Late-time Emission and Dust Formation. RAVI A.P., RHO J., PARK S., et al.
2023ApJ...951...34T 47           X         1 19 3 Supernova 2020wnt: An Atypical Superluminous Supernova with a Hidden Central Engine. TINYANONT S., WOOSLEY S.E., TAGGART K., et al.
2023A&A...678A.209K viz 280           X         6 20 ~ The broad-lined Type-Ic supernova SN 2022xxf and its extraordinary two-humped light curves I. Signatures of H/He-free interaction in the first four months. KUNCARAYAKTI H., SOLLERMAN J., IZZO L., et al.
2024NatAs...8..111F 20       D               2 85 ~ An aspherical distribution for the explosive burning ash of core-collapse supernovae. FANG Q., MAEDA K., KUNCARAYAKTI H., et al.
2024A&A...683A.223S viz 50           X         1 28 ~ 1100 days in the life of the supernova 2018ibb The best pair-instability supernova candidate, to date. SCHULZE S., FRANSSON C., KOZYREVA A., et al.

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