|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| SN 2019stc , the SIMBAD biblio (28 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST11:27:10 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2021ApJ...913..143G |
3369 | T A | X C | 79 | 20 | 17 |
The luminous and double-peaked Type Ic Supernova 2019stc: evidence for multiple energy sources. |
GOMEZ S., BERGER E., HOSSEINZADEH G., et al. | |
| 2021MNRAS.508.4342P | 42 | X | 1 | 26 | 6 | Transitional events in the spectrophotometric regime between stripped envelope and superluminous supernovae. | PRENTICE S.J., INSERRA C., SCHULZE S., et al. | ||
| 2022MNRAS.512L..71C | 511 | T K A | D | X C F | 10 | 2 | ~ | Origin of post-maximum bump in luminous Type Ic supernova 2019stc. | CHUGAI N.N. and UTROBIN V.P. |
| 2022MNRAS.512.4484F | 43 | X | 1 | 24 | 4 | Close, bright, and boxy: the superluminous SN 2018hti. | FIORE A., BENETTI S., NICHOLL M., et al. | ||
| 2022MNRAS.513.6210M | 1007 | K A | S X C F | 21 | 4 | 11 | Variable thermal energy injection from magnetar spin-down as a possible cause of stripped-envelope supernova light-curve bumps. | MORIYA T.J., MURASE K., KASHIYAMA K., et al. | |
| 2022ApJ...935..108S | 17 | D | 1 | 41 | 9 | Powering Luminous Core Collapse Supernovae with Jets. | SOKER N. | ||
| 2022MNRAS.517.4544H | 154 | K A | X | 4 | 5 | 6 | Neutron stars colliding with binary companions: formation of hypervelocity stars, pulsar planets, bumpy superluminous supernovae and Thorne-Żytkow objects. | HIRAI R. and PODSIADLOWSKI P. | |
| 2022A&A...667A..92O | 102 | D | F | 2 | 25 | 2 | Supernova double-peaked light curves from double-nickel distribution. | ORELLANA M. and BERSTEN M.C. | |
| 2022ApJ...941..107G | 570 | D | X | 14 | 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 |
279 | D | X | 7 | 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 |
17 | D | 4 | 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. | ||
|
2023ApJ...950...14R |
218 | X | 5 | 38 | 1 | Near-infrared and Optical Observations of Type Ic SN 2021krf: Luminous Late-time Emission and Dust Formation. | RAVI A.P., RHO J., PARK S., et al. | ||
| 2023ApJ...951...34T | 44 | X | 1 | 19 | 3 | Supernova 2020wnt: An Atypical Superluminous Supernova with a Hidden Central Engine. | TINYANONT S., WOOSLEY S.E., TAGGART K., et al. | ||
| 2023ApJ...951...61D | 279 | D | X C | 6 | 12 | ~ | Magnetar Flare-driven Bumpy Declining Light Curves in Hydrogen-poor Superluminous Supernovae. | DONG X.-F., LIU L.-D., GAO H., 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. | ||
| 2023RAA....23l5002B | 44 | X | 1 | 12 | ~ | The Study of the Physical Properties and Energy Sources of Five Luminous Type Ibc Supernovae. | BAI S.-Y., WANG T., WANG S.-Q., et al. | ||
| 2024MNRAS.527.6473F | 18 | D | 1 | 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. | ||
| 2024Natur.625..253C | 45 | X | 1 | 33 | ~ | A 12.4-day periodicity in a close binary system after a supernova. | CHEN P., GAL-YAM A., SOLLERMAN J., et al. | ||
| 2024ApJ...970L..42Z | 108 | D | X | 3 | 8 | ~ | Bumpy Superluminous Supernovae Powered by a Magnetar-Star Binary Engine. | ZHU J.-P., LIU L.-D., YU Y.-W., et al. | |
| 2024ApJ...973...14C | 134 | X C | 2 | 4 | ~ | Characterization of Supernovae Interacting with Dense Circumstellar Matter with a Flat Density Profile. | CHIBA R. and MORIYA T.J. | ||
| 2024A&A...689A.182K | 45 | X | 1 | 29 | ~ | The enigmatic double-peaked stripped-envelope SN 2023aew. | KANGAS T., KUNCARAYAKTI H., NAGAO T., et al. | ||
| 2024ApJ...977L..41A | 358 | X C | 7 | 16 | ~ | Double “acct”: A Distinct Double-peaked Supernova Matching Pulsational Pair Instability Models. | ANGUS C.R., WOOSLEY S.E., FOLEY R.J., et al. | ||
| 2025ApJ...980..219K | 345 | D | X | 8 | 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. | |
| 2025ApJ...985..172Z | 998 | D | X C | 21 | 10 | ~ | Hydrogen-poor Superluminous Supernovae with Bumpy Light Curves Powered by Precessing Magnetars. | ZHANG B., LI L., DAI Z.-G., et al. | |
| 2025ApJ...989..182G | 140 | X C | 2 | 44 | ~ | Evidence for an Instability-induced Binary Merger in the Double-peaked, Helium-rich Type IIn Supernova 2023zkd. | GAGLIANO A., VILLAR V.A., MATSUMOTO T., et al. | ||
| 2025PASP..137i4101S | 1819 | A | D | X C | 39 | 19 | ~ | Twin Peaks: SN 2021uvy and SN 2022hgk in the Landscape of Double-peaked Stripped Envelope Supernovae. | SHARMA Y., SOLLERMAN J., MEYNARDIE W., et al. |
| 2026A&A...707A.161C | 500 | X C | 9 | 32 | ~ | Unveiling the nature of SN 2022jli: The first double-peaked stripped-envelope supernova showing periodic undulations and dust emission at late times. | CARTIER R., CONTRERAS C., STRITZINGER M., et al. |