SN 2019neq , the SIMBAD biblio

SN 2019neq , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST11:49:36

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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
2019ATel13085....1K 41           X         1 2 ~ HET Spectroscopic Observation and Modeling of SLSN 2019neq. KONYVES-TOTH R., VINKO J., THOMAS B.P., et al.
2019ATel13184....1T 81           X         2 1 ~ Extremely fast spectral evolution of SLSN 2019neq. THOMAS B.P., KONYVES-TOTH R., VINKO J., et al.
2020ApJ...900...73K viz 4363 T   A D S   X C       104 11 ~ Comparative spectral analysis of the superluminous supernova 2019neq. KONYVES-TOTH R., THOMAS B.P., VINKO J., et al.
2020ApJ...904...74G 16       D               1 145 ~ FLEET: a redshift-agnostic machine learning pipeline to rapidly identify hydrogen-poor superluminous supernovae. GOMEZ S., BERGER E., BLANCHARD P.K., et al.
2021ApJ...909...24K 142       D     X         4 93 ~ Photospheric velocity gradients and ejecta masses of hydrogen-poor superluminous supernovae: proxies for distinguishing between fast and slow events. KONYVES-TOTH R. and VINKO J.
2021MNRAS.502.1678K 42           X         1 51 12 SN 2020ank: a bright and fast-evolving H-deficient superluminous supernova. KUMAR A., KUMAR B., PANDEY S.B., et al.
2021MNRAS.507.1229P 42           X         1 39 18 Photometric, polarimetric, and spectroscopic studies of the luminous, slow-decaying Type Ib SN 2012au. PANDEY S.B., KUMAR A., KUMAR B., et al.
2022ApJ...933...14H viz 60       D     X         2 35 28 Bumpy Declining Light Curves Are Common in Hydrogen-poor Superluminous Supernovae. HOSSEINZADEH G., BERGER E., METZGER B.D., et al.
2022ApJ...940...69K 145       D     X         4 32 2 Premaximum Spectroscopic Diversity of Hydrogen-poor Superluminous Supernovae. KONYVES-TOTH R.
2022ApJ...941..107G 43           X         1 238 16 Luminous Supernovae: Unveiling a Population between Superluminous and Normal Core-collapse Supernovae. GOMEZ S., BERGER E., NICHOLL M., et al.
2023ApJ...943...41C viz 235       D     X         6 104 17 The Hydrogen-poor Superluminous Supernovae from the Zwicky Transient Facility Phase I Survey. I. Light Curves and Measurements. CHEN Z.H., YAN L., KANGAS T., et al.
2023ApJ...943...42C viz 714       D     X C       16 88 22 The Hydrogen-poor Superluminous Supernovae from the Zwicky Transient Facility Phase I Survey. II. Light-curve Modeling and Characterization of Undulations. CHEN Z.H., YAN L., KANGAS T., et al.
2023A&A...674A..81P 757       D S   X C       16 20 5 Polarimetry of hydrogen-poor superluminous supernovae. PURSIAINEN M., LELOUDAS G., CIKOTA A., et al.
2023MNRAS.524.3559C 17       D               1 56 ~ Metallicity beats sSFR: the connection between superluminous supernova host galaxy environments and the importance of metallicity for their production. CLELAND C., McGEE S.L. and NICHOLL M.
2023ApJ...954...44K 17       D               1 29 ~ Type W and Type 15bn Subgroups of Hydrogen-poor Superluminous Supernovae: Premaximum Diversity, Postmaximum Homogeneity? KONYVES-TOTH R. and SELI B.
2024MNRAS.527.6473F 5062 T K A D S   X C F     110 37 ~ Detailed spectrophotometric analysis of the superluminous and fast evolving
SN 2019neq. 		FIORE A., BENETTI S., TARTAGLIA L., et al.
2024ApJ...961..169H 18       D               2 110 ~ An Extensive Hubble Space Telescope Study of the Offset and Host Light Distributions of Type I Superluminous Supernovae. HSU B., BLANCHARD P.K., BERGER E., et al.
2024MNRAS.535..471G 287       D S   X         6 274 ~ The Type I superluminous supernova catalogue I: light-curve properties, models, and catalogue description. GOMEZ S., NICHOLL M., BERGER E., et al.
2025ApJ...980..219K 532       D     X         12 137 ~ The Bolometric Light-curve Modeling of 98 Type I Superluminous Supernovae Using the Magnetar- and the Circumstellar Interaction Models Reveals Surprisingly High Ejecta Masses. KONYVES-TOTH R.
2026ApJ...999...59B 20       D               2 34 ~ Hydrogen-poor Superluminous Supernovae in the Nebular Phase: Spectral Diversity Due to Ejecta Ionization as a Probe of the Power Source. BLANCHARD P.K., BERGER E., GOMEZ S., et al.

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