GRB 130919A , the SIMBAD biblio

GRB 130919A , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST01:13:36


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Title First 3 Authors
2013GCN.15232....1K 77 T                   1 ~ GRB 130919A: Swift detection of a burst. KRIMM H.A., BREEVELD A.A., BURROWS D.N., et al.
2013GCN.15234....1L 77 T                   1 ~ GRB 130919A, Swift-BAT refined analysis. LIEN A.Y., BARTHELMY S.D., CUMMINGS J.R., et al.
2013GCN.15235....1T 77 T                   1 ~ GRB 130919A: skynet PROMPT-CTIO optical upper limits. TROTTER A., REICHART D., HAISLIP J., et al.
2013GCN.15238....1L 77 T                   1 ~ Fermi trigger 401326696: MASTER prompt optical observations. LEVATO H., SAFFE C., MALLAMACI C., et al.
2014ApJ...787...90G viz 15       D               1 484 27 Uncovering the intrinsic variability of gamma-ray bursts. GOLKHOU V.Z. and BUTLER N.R.
2016ApJ...829....7L viz 16       D               1 1010 215 The third Swift burst alert telescope gamma-ray burst catalog. LIEN A., SAKAMOTO T., BARTHELMY S.D., et al.
2018ApJ...866...97B viz 16       D               1 629 1 Statistical study of the Swift X-ray flash and X-ray rich Gamma-ray bursts. BI X., MAO J., LIU C., et al.
2020ApJ...893...77W viz 16       D               1 3281 34 A comprehensive statistical study of gamma-ray bursts. WANG F., ZOU Y.-C., LIU F., et al.
2020ApJ...896L..20J viz 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 viz 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.
2022ApJ...925..152U viz 17       D               1 478 ~ The Second AGILE MCAL Gamma-Ray Burst Catalog: 13 yr of Observations. URSI A., ROMANI M., VERRECCHIA F., et al.
2023A&A...671A.112C viz 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.

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