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| SN 2020tcw , the SIMBAD biblio (13 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST04:32:27 |
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More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2021MNRAS.508...44M | 43 | X | 1 | 9 | 10 | ALMA and NOEMA constraints on synchrotron nebular emission from embryonic superluminous supernova remnants and radio-gamma-ray connection. | MURASE K., OMAND C.M.B., COPPEJANS D.L., et al. | ||
| 2021ATel14418....1C | 209 | T | X | 4 | 3 | ~ |
Radio detection of the hydrogen-poor super-luminous supernova 2020tcw at 64 days post discovery. |
COPPEJANS D.L., MATTHEWS D., MARGUTTI R., et al. | |
| 2021ATel14580....1M | 334 | T | X | 7 | 1 | ~ |
X-ray detection of the SLSN-I 2020tcw. |
MATTHEWS D., MARGUTTI R., COPPEJANS D., et al. | |
| 2022MNRAS.511.5948P | 43 | X | 1 | 22 | 5 | Post maximum light and late time optical imaging polarimetry of type I superluminous supernova 2020znr. | POIDEVIN F., OMAND C.M.B., PEREZ-FOURNON I., et al. | ||
| 2023A&A...670A...7W | 44 | X | 1 | 16 | 6 | SN 2020qlb: A hydrogen-poor superluminous supernova with well-characterized light curve undulations. | WEST S.L., LUNNAN R., OMAND C.M.B., et al. | ||
| 2023ApJ...949..114G | 17 | D | 1 | 67 | 3 | The First Two Years of FLEET: An Active Search for Superluminous Supernovae. | GOMEZ S., BERGER E., BLANCHARD P.K., et al. | ||
| 2023A&A...674A..81P | 714 | D | S X C | 15 | 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. | ||
| 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. | ||
2024A&A...683A.223S 
|
45 | X | 1 | 28 | ~ | 1100 days in the life of the supernova 2018ibb The best pair-instability supernova candidate, to date. | SCHULZE S., FRANSSON C., KOZYREVA A., 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. | |
| 2025ApJ...980..219K | 19 | D | 1 | 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 | 170 | D | X | 4 | 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. |
