iPTF 13beo , the SIMBAD biblio

iPTF 13beo , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.7 - 2021.06.15CEST07:54:56


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Title First 3 Authors
2020ApJ...889..170G 93             C       1 24 ~ Flash ionization signatures in the Type Ibn supernova SN 2019uo. GANGOPADHYAY A., MISRA K., HIRAMATSU D., et al.
2020ApJ...900...83W 47           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.492.2208C 93               F     1 39 ~ LSQ13ddu: a rapidly evolving stripped-envelope supernova with early circumstellar interaction signatures. CLARK P., MAGUIRE K., INSERRA C., et al.
2019ApJ...871L...9H 18       D               1 32 ~ Type Ibn supernovae may not all come from massive stars. HOSSEINZADEH G., McCULLY C., ZABLUDOFF A.I., et al.
2017A&A...602A..93K viz 85             C       1 19 3 OGLE-2014-SN-131: A long-rising Type Ibn supernova from a massive progenitor. KARAMEHMETOGLU E., TADDIA F., SOLLERMAN J., et al.
2017ApJ...836..158H 358       D     X         9 37 12 Type Ibn supernovae show photometric homogeneity and spectral diversity at maximum light. HOSSEINZADEH G., ARCAVI I., VALENTI S., et al.
2016A&A...596A..67R 42           X         1 60 9 SN 2012aa: A transient between Type Ibc core-collapse and superluminous supernovae. ROY R., SOLLERMAN J., SILVERMAN J.M., et al.
2016ApJ...821...57D viz 42           X         1 43 29 The double-peaked SN 2013ge: a Type Ib/c SN with an asymmetric mass ejection or an extended progenitor envelope. DROUT M.R., MILISAVLJEVIC D., PARRENT J., et al.
2016ApJ...824..100M 100       D     X         3 21 6 Circumstellar and explosion properties of type ibn supernovae. MORIYA T.J. and MAEDA K.
2016MNRAS.456..853P 476       D     X C       11 47 20 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.
2016MNRAS.461.3057S 42           X         1 35 17 SN 2015U: a rapidly evolving and luminous Type Ibn supernova. SHIVVERS I., ZHENG W., MAUERHAN J., et al.
2016PASP..128k4502C 86             C       2 8 23 Intermediate Palomar Transient Factory: realtime image subtraction pipeline. CAO Y., NUGENT P.E. and KASLIWAL M.M.
2015MNRAS.449.1921P viz 330           X C       7 24 27 Massive stars exploding in a He-rich circumstellar medium - IV. Transitional Type Ibn supernovae. PASTORELLO A., BENETTI S., BROWN P.J., et al.
2015MNRAS.449.1954P 140       D     X C       3 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.
2015MNRAS.453.3649P viz 41           X         1 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 82           X         2 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.
2014A&A...564A..83M 43           X         1 8 16 Mass loss of massive stars near the Eddington luminosity by core neutrino emission shortly before their explosion. MORIYA T.J.
2014ApJ...788..193N 89           X         2 6 52 Supernovae with two peaks in the optical light curve and the signature of progenitors with low-mass extended envelopes. NAKAR E. and PIRO A.L.
2014ApJ...794...23D viz 83           X         2 29 76 Rapidly evolving and luminous transients from Pan-STARRS1. DROUT M.R., CHORNOCK R., SODERBERG A.M., et al.
2014MNRAS.441.2230H 41           X         1 100 33 Environments of interacting transients: impostors and Type IIn supernovae. HABERGHAM S.M., ANDERSON J.P., JAMES P.A., et al.
2014MNRAS.443..671G 1895 T K A     X C F     44 13 26
iPTF13beo: the double-peaked light curve of a Type Ibn supernova discovered shortly after explosion.
GORBIKOV E., GAL-YAM A., OFEK E.O., et al.

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2021.06.15-07:54:57

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