ASASSN -14ms , the SIMBAD biblio

ASASSN -14ms , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST08:08:11

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2014ATel.6853....1K 116           X         3 2 2 ASAS-SN Discovery of A Possible Extreme Luminosity Transient in SDSS J130408.52+521846.4. KIYOTA S., HOLOIEN T.W.-S., STANEK K.Z., et al.
2017MNRAS.464.2672H viz 56       D     X         2 171 29 The ASAS-SN bright supernova catalogue - I. 2013-2014. HOLOIEN T.W.-S., STANEK K.Z., KOCHANEK C.S., et al.
2018MNRAS.475.2344V 2368 T K A D     X C F     57 19 7 The highly luminous Type Ibn supernova
ASASSN-14ms. 		VALLELY P.J., PRIETO J.L., STANEK K.Z., et al.
2019ApJ...871L...9H 57       D     X         2 32 11 Type Ibn supernovae may not all come from massive stars. HOSSEINZADEH G., McCULLY C., ZABLUDOFF A.I., et al.
2019A&A...624A.143K 42           X         1 63 71 Highly luminous supernovae associated with gamma-ray bursts. I. GRB 111209A/SN 2011kl in the context of stripped-envelope and superluminous supernovae. KANN D.A., SCHADY P., OLIVARES F.E., et al.
2020ApJ...900...83W 82             C       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.
2021ApJ...910...42X viz 85             C       1 23 25 The peculiar transient AT2018cow: a possible origin of a Type Ibn/IIn supernova. XIANG D., WANG X., LIN W., et al.
2021MNRAS.503.3931T viz 17       D               1 248 41 Core-collapse, superluminous, and gamma-ray burst supernova host galaxy populations at low redshift: the importance of dwarf and starbursting galaxies. TAGGART K. and PERLEY D.A.
2021ApJ...917...97W viz 3327 T   A S   X C       77 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.
2022ApJ...930..127G viz 43           X         1 35 3 Evolution of a Peculiar Type Ibn Supernova SN 2019wep. GANGOPADHYAY A., MISRA K., HOSSEINZADEH G., et al.
2022ApJ...933..196H viz 43           X         1 32 13 Investigating the Nature of the Luminous Ambiguous Nuclear Transient ASASSN-17jz. HOLOIEN T.W.-S., NEUSTADT J.M.M., VALLELY P.J., 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 131           X C       2 21 1 The Type Ibn Supernova 2019kbj: Indications for Diversity in Type Ibn Supernova Progenitors. BEN-AMI T., ARCAVI I., NEWSOME M., et al.
2024A&A...691A.156W viz 45           X         1 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 108       D       C       4 188 ~ Multifilter UV to Near-infrared Data-driven Light-curve Templates for Stripped-envelope Supernovae. KHAKPASH S., BIANCO F.B., MODJAZ M., et al.
2025A&A...696A.103E 47           X         1 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 65       D     X         2 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.
2025A&A...703A..34P viz 93           X         2 37 ~ Supernova rates and luminosity functions from ASAS-SN II. 2014-2017 core-collapse supernovae and their subtypes. PESSI T., DESAI D.D., PRIETO J.L., et al.
2026A&A...707A.157C viz 150           X         3 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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