OGLE 2012-SN-6 , the SIMBAD biblio

OGLE 2012-SN-6 , the SIMBAD biblio (42 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST14:20:43


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Title First 3 Authors
2012ATel.4495....1W 38           X         1 21 5 18 supernovae candidates detected by the OGLE-IV survey. WYRZYKOWSKI L., UDALSKI A. and KOZLOWSKI S.
2013ATel.4734....1P 38           X         1 10 5 Spectroscopic classification of optical transients at Las Campanas Observatory. PRIETO J.L. and MORRELL N.
2015MNRAS.449.1921P viz 195           X C       4 24 38 Massive stars exploding in a He-rich circumstellar medium - IV. Transitional Type Ibn supernovae. PASTORELLO A., BENETTI S., BROWN P.J., et al.
2015MNRAS.449.1941P viz 2847 T K A D     X C       72 14 11 Massive stars exploding in a He-rich circumstellar medium - V. Observations of the slow-evolving SN Ibn
OGLE-2012-SN-006.
PASTORELLO A., WYRZYKOWSKI L., VALENTI S., et al.
2015MNRAS.449.1954P 211       D     X C       5 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.
2015A&A...579A..40S viz 80               F     1 49 256 PESSTO: survey description and products from the first data release by the Public ESO Spectroscopic Survey of Transient Objects. SMARTT S.J., VALENTI S., FRASER M., et al.
2014AcA....64..197W viz 54       D     X         2 247 28 OGLE-IV real-time transient search. WYRZYKOWSKI L., KOSTRZEWA-RUTKOWSKA Z., KOZLOWSKI S., et al.
2015MNRAS.453.3649P viz 117           X C       2 20 13 Massive stars exploding in a He-rich circumstellar medium - VII. The metamorphosis of ASASSN-15ed from a narrow line Type Ibn to a normal Type Ib Supernova. PASTORELLO A., PRIETO J.L., ELIAS-ROSA N., et al.
2015MNRAS.454.4293P 39           X         1 15 8 Massive stars exploding in a He-rich circumstellar medium - VIII. PSN J07285387+3349106, a highly reddened supernova Ibn. PASTORELLO A., TARTAGLIA L., ELIAS-ROSA N., et al.
2016MNRAS.456..853P 488       D     X C       12 47 33 Massive stars exploding in a He-rich circumstellar medium - IX. SN 2014av, and characterization of Type Ibn SNe. PASTORELLO A., WANG X.-F., CIABATTARI F., et al.
2016ApJ...824..100M 118           X         3 21 6 Circumstellar and explosion properties of type ibn supernovae. MORIYA T.J. and MAEDA K.
2017ApJ...836..158H 335       D     X         9 37 82 Type Ibn supernovae show photometric homogeneity and spectral diversity at maximum light. HOSSEINZADEH G., ARCAVI I., VALENTI S., et al.
2017A&A...602A..93K viz 199           X C       4 19 3 OGLE-2014-SN-131: A long-rising Type Ibn supernova from a massive progenitor. KARAMEHMETOGLU E., TADDIA F., SOLLERMAN J., et al.
2018ApJ...855....2Q 242           X         6 63 93 Spectra of hydrogen-poor superluminous supernovae from the Palomar Transient Factory. QUIMBY R.M., DE CIA A., GAL-YAM A., et al.
2018MNRAS.475.2344V 201           X   F     4 19 7 The highly luminous Type Ibn supernova ASASSN-14ms. VALLELY P.J., PRIETO J.L., STANEK K.Z., et al.
2020MNRAS.492.2208C 41           X         1 39 ~ LSQ13ddu: a rapidly evolving stripped-envelope supernova with early circumstellar interaction signatures. CLARK P., MAGUIRE K., INSERRA C., et al.
2020ApJ...889..170G 206           X C       4 24 17 Flash ionization signatures in the Type Ibn supernova SN 2019uo. GANGOPADHYAY A., MISRA K., HIRAMATSU D., et al.
2020ApJ...900...83W 41           X         1 15 ~ Exploring the energy sources powering the light curve of the Type Ibn supernova PS15dpn and the mass-loss history of the SN progenitor. WANG S.-Q. and LI L.
2020MNRAS.499.1450P 206           X C F     3 24 13 SN 2018gjx reveals that some SNe Ibn are SNe IIb exploding in dense circumstellar material. PRENTICE S.J., MAGUIRE K., BOIAN I., et al.
2021ApJ...914..125G 2048     A D S   X C       48 22 ~ The study of dust formation of four Type Ibn supernovae. GAN W.-P., WANG S.-Q. and LIANG E.-W.
2021ApJ...917...97W viz 84             C       1 27 3 ASASSN-14ms: the most energetic known explosion of a Type Ibn supernova and its physical origin. WANG X., LIN W., ZHANG J., et al.
2021A&A...652A.136K viz 42           X         1 18 8 SN 2020bqj: A Type Ibn supernova with a long-lasting peak plateau. KOOL E.C., KARAMEHMETOGLU E., SOLLERMAN J., et al.
2021MNRAS.506.4819P 84           X         2 21 3 SN 2019hcc: a Type II supernova displaying early O II lines. PARRAG E., INSERRA C., SCHULZE S., et al.
2022A&A...658A.130D 85           X         2 12 9 Helium stars exploding in circumstellar material and the origin of Type Ibn supernovae. DESSART L., HILLIER D.J. and KUNCARAYAKTI H.
2022ApJ...927...25M 130           X C       2 9 18 Properties of Type Ibn Supernovae: Implications for the Progenitor Evolution and the Origin of a Population of Rapid Transients. MAEDA K. and MORIYA T.J.
2022ApJ...928...77L 43           X         1 69 ~ Using the Optical-NIR Spectral Energy Distributions to Search for the Evidence of Dust Formation of 66 Supernovae. LI J.-Y., WANG S.-Q., GAN W.-P., et al.
2022ApJ...930..127G viz 213           X C       4 35 3 Evolution of a Peculiar Type Ibn Supernova SN 2019wep. GANGOPADHYAY A., MISRA K., HOSSEINZADEH G., et al.
2022MNRAS.514.5686P 17       D               2 87 9 Oxygen and calcium nebular emission line relationships in core-collapse supernovae and Ca-rich transients. PRENTICE S.J., MAGUIRE K., SIEBENALER L., et al.
2022A&A...666A..30P 43           X         1 43 14 SN 2018bsz: A Type I superluminous supernova with aspherical circumstellar material. PURSIAINEN M., LELOUDAS G., PARASKEVA E., et al.
2022ApJ...939..105B viz 145       D S   X         3 121 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.
2023ApJ...946...30B viz 87             C       1 21 1 The Type Ibn Supernova 2019kbj: Indications for Diversity in Type Ibn Supernova Progenitors. BEN-AMI T., ARCAVI I., NEWSOME M., et al.
2023NatAs...7..779L 174           X C       3 16 ~ A superluminous supernova lightened by collisions with pulsational pair-instability shells. LIN W., WANG X., YAN L., et al.
2024ApJ...961...67T 90           X         2 18 ~ Simulating Hydrogen-poor Interaction-powered Supernovae with CHIPS. TAKEI Y., TSUNA D., KO T., et al.
2024ApJ...967...13S 45           X         1 10 ~ On the Formation of the W-shaped O II Lines in Spectra of Type I Superluminous Supernovae. SAITO S., TANAKA M., MAZZALI P.A., et al.
2024A&A...687A.108G viz 18       D               1 1820 ~ Narrow absorption lines from intervening material in supernovae I. Measurements and temporal evolution. GONZALEZ-GAITAN S., GUTIERREZ C.P., ANDERSON J.P., et al.
2024A&A...691A.156W viz 448           X   F     9 35 ~ Massive stars exploding in a He-rich circumstellar medium X. Flash spectral features in the Type Ibn SN 2019cj and observations of SN 2018jmt. WANG Z.-Y., PASTORELLO A., MAEDA K., et al.
2024ApJS..275...37K 242       D     X         6 188 ~ Multifilter UV to Near-infrared Data-driven Light-curve Templates for Stripped-envelope Supernovae. KHAKPASH S., BIANCO F.B., MODJAZ M., et al.
2025MNRAS.536.3588W 47           X         1 15 ~ SN 2023tsz: a helium-interaction-driven supernova in a very low-mass galaxy. WARWICK B., LYMAN J., PURSIAINEN M., et al.
2025MNRAS.537.2898G 140           X   F     2 36 ~ SN 2021foa: the bridge between SN IIn and Ibn. GANGOPADHYAY A., DUKIYA N., MORIYA T.J., et al.
2025A&A...696A.103E 140           X C       2 32 ~ Mass-transferring binary stars as progenitors of interacting hydrogen-free supernovae. ERCOLINO A., JIN H., LANGER N., et al.
2025A&A...700A.156W viz 159       D     X         4 43 ~ Massive stars exploding in a He-rich circumstellar medium XI. Diverse evolution of five Ibn SNe 2020nxt, 2020taz, 2021bbv, 2023utc, and 2024aej. WANG Z.-Y., PASTORELLO A., CAI Y.-Z., et al.
2026A&A...707A.157C viz 50           X         1 30 ~ Massive stars exploding in a He-rich circumstellar medium XII. SN 2024acyl: A fast, linearly declining Type Ibn supernova with early flash-ionisation features. CAI Y.-Z., PASTORELLO A., MAEDA K., et al.

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