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| SN 2018bym , the SIMBAD biblio (18 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST14:22:10 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2018ATel11714....1B | 80 | T | X | 1 | 2 | ~ |
Classification of AT2018bym as a Type I Superluminous Supernova. |
BLANCHARD P., GOMEZ S., BERGER E., et al. | |
|
2020ApJ...895...32F |
58 | D | X | 2 | 1494 | 104 | The Zwicky Transient Facility Bright Transient Survey. I. Spectroscopic classification and the redshift completeness of local galaxy catalogs. | FREMLING C., MILLER A.A., SHARMA Y., et al. | |
|
2020ApJ...901...61L |
2265 | A | D | S X C | 54 | 27 | 32 | Four (super)luminous supernovae from the first months of the ZTF survey. | LUNNAN R., YAN L., PERLEY D.A., 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. | ||
| 2021MNRAS.500.5142F | 17 | D | 1 | 113 | 29 | From core collapse to superluminous: the rates of massive stellar explosions from the Palomar Transient Factory. | FROHMAIER C., ANGUS C.R., VINCENZI M., et al. | ||
|
2022ApJ...933...14H |
315 | D | X C | 7 | 35 | 28 | Bumpy Declining Light Curves Are Common in Hydrogen-poor Superluminous Supernovae. | HOSSEINZADEH G., BERGER E., METZGER B.D., et al. | |
| 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 |
17 | D | 9 | 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 |
366 | D | X C | 8 | 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. | |
| 2023MNRAS.518.6123A | 44 | X | 1 | 4 | 3 | Rapid decline in the lightcurves of luminous supernovae by jet-driven bipolar explosions. | AKASHI M., MICHAELIS A. and SOKER N. | ||
| 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. | ||
| 2024MNRAS.527.6473F | 63 | D | X | 2 | 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 | 332 | D | S X | 7 | 274 | ~ | The Type I superluminous supernova catalogue I: light-curve properties, models, and catalogue description. | GOMEZ S., NICHOLL M., BERGER E., et al. | |
|
2024A&A...691A.181P |
179 | X C | 3 | 4 | ~ | ELEPHANT: ExtragaLactic alErt Pipeline for Hostless AstroNomical Transients. | PESSI P.J., DURGESH R., NAKAZONO L., et al. | ||
| 2025ApJ...980..219K | 625 | D | X C | 13 | 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. | |
| 2025MNRAS.541.2674A | 19 | D | 1 | 60 | ~ | The Type I superluminous supernova catalogue - II. Spectroscopic evolution in the photospheric phase, velocity measurements, and constraints on diversity. | AAMER A., NICHOLL M., GOMEZ S., et al. | ||
| 2026ApJ...999...59B | 120 | D | X | 3 | 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. |