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| GRB 170306A , the SIMBAD biblio (12 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST23:39:21 |
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| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2017GCN.20819....1M | 79 | T | 1 | ~ |
GRB 170306A: Swift detection of a burst. |
MARKWARDT C.B., D'ELIA V., KENNEA J.A., et al. | |||
| 2017GCN.20820....1G | 79 | T | 1 | ~ |
GRB 170306A: LCO Cerro Tololo observations. |
GUIDORZI C., KOBAYASHI S., STEELE I.A., et al. | |||
| 2017GCN.20822....1S | 79 | T | 1 | ~ |
GRB 170306A: GROND observations. |
SCHADY P., WISEMAN P. and BOLMER J. | |||
| 2017GCN.20823....1E | 79 | T | 1 | ~ |
GRB 170306A: Swift/UVOT Upper Limits. |
EMERY S.W.K. and MARKWARDT C.B. | |||
| 2017GCN.20828....1D | 79 | T | 1 | ~ |
GRB 170306A: Swift-XRT refined Analysis. |
D'AVANZO P., D'ELIA V., D'AI A., et al. | |||
| 2017GCN.20829....1S | 79 | T | 1 | ~ |
GRB 170306A, Swift-BAT refined analysis. |
SAKAMOTO T., BARTHELMY S.D., CUMMINGS J.R., et al. | |||
| 2017GCN.20843....1S | 79 | T | 1 | ~ |
GRB 170306A: GROND afterglow detection. |
SCHADY P. | |||
| 2017GCN.20844....1B | 79 | T | 1 | ~ |
GRB170306A: SALT observations. |
BUCKLEY D.A.H., MARTIN-CARRILLO A., RAZZAQUE 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. | ||
| 2023A&A...672A.102L | 17 | D | 1 | 11 | 8 | Neutrino search from γ-ray bursts during the prompt and X-ray afterglow phases using 10 years of IceCube public data. | LUCARELLI F., OGANESYAN G., MONTARULI T., et al. |
