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| Fermi bn180410336 , the SIMBAD biblio (12 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST09:55:42 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2018GCN.22620....1G | 80 | T | 1 | ~ |
GRB 180410A: Swift detection of a burst or a Galactic transient. |
GROPP J.D., DEICH A., EVANS P.A., et al. | |||
| 2018GCN.22622....1E | 80 | T | 1 | ~ |
GRB 180410A: Enhanced Swift-XRT position. |
EVANS P.A., GOAD M.R., OSBORNE J.P., et al. | |||
| 2018GCN.22623....1I | 80 | T | 1 | ~ |
GRB 180410A: MITSuME Akeno optical upper limits. |
ITOH R., MURATA K.L., TACHIBANA Y., et al. | |||
| 2018GCN.22627....1M | 80 | T | 1 | ~ |
GRB 180410A: Swift/UVOT Upper Limits. |
MARSHALL F.E. and GROPP J.D. | |||
| 2018GCN.22628....1L | 80 | T | 1 | ~ |
GRB 180410A: Swift-BAT refined analysis. |
LIEN A.Y., BARTHELMY S.D., CUMMINGS J.R., et al. | |||
| 2018GCN.22629....1E | 80 | T | 1 | ~ |
GRB 180410A: Swift-XRT refined Analysis. |
EVANS P.A., GIBSON S.L., LIU Z., et al. | |||
| 2018GCN.22631....1W | 80 | T | 1 | ~ |
GRB 180410A: RATIR Optical Observations. |
WATSON A.M., BUTLER N., KUTYREV A., et al. | |||
| 2018GCN.22636....1B | 80 | T | 1 | ~ |
GRB 180410A: Fermi GBM observation. |
BISSALDI E. | |||
|
2020ApJ...893...46V |
16 | D | 1 | 2357 | 157 | The fourth Fermi-GBM Gamma-ray Burst catalog: a decade of data. | VON KIENLIN A., MEEGAN C.A., PACIESAS W.S., et al. | ||
|
2020ApJ...896L..20J |
16 | D | 1 | 1320 | 28 | An unambiguous separation of gamma-ray bursts into two classes from prompt emission alone. | JESPERSEN C.K., SEVERIN J.B., STEINHARDT C.L., et al. | ||
|
2021ApJ...911...20T |
17 | D | 1 | 1354 | 14 | A comprehensive power spectral density analysis of astronomical time series. II. The Swift/BAT long gamma-ray bursts. | TARNOPOLSKI M. and MARCHENKO V. | ||
|
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. |