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| GRB 190320A , the SIMBAD biblio (12 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST16:28:37 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2019GCN.23973....1G | 81 | T | 1 | ~ |
GRB 190320A: Swift detection of a burst. |
GROPP J.D., KRIMM H.A., LIEN A.Y., et al. | |||
| 2019GCN.23974....1K | 81 | T | 1 | ~ |
GRB 190320A: Swift-XRT observations. |
KENNEA J.A., CUSUMANO G., PERRI M., et al. | |||
| 2019GCN.23976....1L | 81 | T | 1 | ~ |
GRB190320A: MASTER OT detection. |
LIPUNOV V., GORBOVSKOY E., TYURINA N., et al. | |||
| 2019GCN.23977....1O | 81 | T | 1 | ~ |
GRB 190320A: Enhanced Swift-XRT position. |
OSBORNE J.P., BEARDMORE A.P., EVANS P.A., et al. | |||
| 2019GCN.23979....1L | 81 | T | 1 | ~ |
GRB190320A: MASTER GRB counterpart decay. |
LIPUNOV V., GORBOVSKOY E., TYURINA N., et al. | |||
| 2019GCN.23980....1K | 81 | T | 1 | ~ |
GRB 190320A: Swift-BAT refined analysis. |
KRIMM H.A., BARTHELMY S.D., CUMMINGS J.R., et al. | |||
| 2019GCN.23981....1P | 81 | T | 1 | ~ |
GRB 190320A: Swift-XRT refined Analysis. |
PAGE K.L., D'ELIA V., D'AI A., et al. | |||
| 2019GCN.23982....1M | 81 | T | 1 | ~ |
GRB 190320A: Swift/UVOT Upper Limits. |
MARSHALL F.E. and GROPP J.D. | |||
| 2020ApJ...895...40G | 16 | D | 1 | 26 | ~ | Evaluation of automated Fermi GBM localizations of Gamma-ray bursts. | GOLDSTEIN A., FLETCHER C., VERES P., 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. |