|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| SN 2023pel , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST10:15:54 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2024ApJ...960L..18S | 2536 | T A | X C | 55 | 11 | ~ |
Characterizing the Ordinary Broad-line Type Ic SN 2023pel from the Energetic GRB 230812B. |
SRINIVASARAGAVAN G.P., SWAIN V., O'CONNOR B., et al. | |
| 2024MNRAS.530....1H | 1254 | T A | D | S X C F | 25 | 23 | ~ |
Multiband analyses of the bright GRB 230812B and the associated SN2023pel. |
HUSSENOT-DESENONGES T., WOUTERS T., GUESSOUM N., et al. |
| 2025A&A...698A..78R | 3154 | T K A | X C | 66 | 18 | ~ |
A magnetar powers the luminous supernova 2023pel, which is associated with a long gamma-ray burst. |
ROMAN AGUILAR L.M., SAEZ M.M., ERTINI K., et al. | |
| 2025ApJ...988L..60S | 187 | X C | 3 | 17 | ~ | EP250108a/SN 2025kg: A Jet-driven Stellar Explosion Interacting with Circumstellar Material. | SRINIVASARAGAVAN G.P., HAMIDANI H., SCHROEDER G., et al. | ||
| 2025ApJ...993...20D | 19 | D | 1 | 556 | ~ | A Statistical Study of the Gamma-Ray Burst and Supernova Association. | DONG X.-F., HUANG Y.-F., ZHANG Z.-B., et al. | ||
| 2025A&A...702L..18R | 746 | A | D | X C | 16 | 6 | ~ | Hydrodynamical modeling of SN 2025kg associated with the fast X-ray transient EP250108a. | ROMAN AGUILAR L.M. and BERSTEN M.C. |
| 2026A&A...705A.227M | 100 | X | 2 | 8 | ~ | Broad-band modelling of the GRB 230812B afterglow: Implications for very-high-energy γ-ray detections with IACTs. | MOHNANI S., BANERJEE B., MICELI D., et al. | ||
| 2026ApJ...998..188K | 20 | D | 1 | 35 | ~ | Unifying the Circumstellar Environment in Broad-lined Type Ic Radio Supernovae toward Off-axis Gamma-Ray Burst Exploration. | KUSAFUKA Y., MATSUOKA T. and SAWADA R. |