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| GRB 210725A , the SIMBAD biblio (12 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST13:38:27 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2021GCN.30501....1B | 84 | T | 1 | ~ |
GRB 210725A: Swift detection of a burst. |
BERNARDINI M.G., D'AVANZO P., KLINGLER N.J., et al. | |||
| 2021GCN.30503....1Z | 84 | T | 1 | ~ |
GRB 210725A: KAIT Optical Upper Limit. |
ZHENG W. and FILIPPENKO A.V. | |||
| 2021GCN.30507....1T | 84 | T | 1 | ~ |
GRB 210725A: CALET Gamma-Ray Burst Monitor detection. |
TORII S., YOSHIDA A., SAKAMOTO T., et al. | |||
| 2021GCN.30509....1N | 84 | T | 1 | ~ |
GRB 210725A: MITSuME Akeno optical upper limits. |
NIWANO M., HOSOKAWA R., MURATA K.L., et al. | |||
| 2021GCN.30514....1L | 84 | T | 1 | ~ |
GRB 210725A: Swift-BAT refined analysis. |
LIEN A.Y., BARTHELMY S.D., BERNARDINI M.G., et al. | |||
| 2021GCN.30517....1P | 84 | T | 1 | ~ |
GRB 210725A: Swift-XRT refined Analysis. |
PERRI M., D'ELIA V., D'AI A., et al. | |||
| 2021GCN.30519....1P | 84 | T | 1 | ~ |
GRB 210725A: Fermi GBM detection. |
POOLAKKIL S. and MEEGAN C. | |||
| 2021GCN.30527....1S | 84 | T | 1 | ~ |
GRB 210725A: Swift/UVOT Upper Limits. |
SIEGEL M.H. and BERNARDINI M.G. | |||
| 2021GCN.30530....1P | 84 | T | 1 | ~ |
GRB 210725A: AbAO optical upper limit. |
PANKOV N., INASARIDZE R.Y., POZANENKO A., et al. | |||
|
2023A&A...671A.112C |
17 | D | 1 | 1469 | 4 | GRB minimum variability timescale with Insight-HXMT and Swift Implications for progenitor models, dissipation physics, and GRB classifications. | CAMISASCA A.E., GUIDORZI C., AMATI L., et al. | ||
| 2024MNRAS.531.2775L | 18 | D | 1 | 75 | ~ | An evaluation of the BALROG and RoboBA algorithms for determining the position of Fermi/GBM GRBs. | LOPEZ K.O.C., WATSON A.M., LEE W.H., et al. | ||
| 2025ApJ...979...11X | 65 | D | X | 2 | 45 | ~ | Constraining the Gamma-Ray Burst Jet Opening Angle Based on the Very Steep Decay Phase. | XU Q., LIU D.-J. and ZOU Y.-C. |