GRB 150925A , the SIMBAD biblio

GRB 150925A , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST17:34:49


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Title First 3 Authors
2015GCN.18365....1R 78 T                   1 ~ GRB 150925A: Swift detection of a burst. RACUSIN J.L., D'AI A., MASELLI A., et al.
2015GCN.18366....1O 78 T                   1 ~ GRB 150925A: Enhanced Swift-XRT position. OSBORNE J.P., BEARDMORE A.P., EVANS P.A., et al.
2015GCN.18367....1M 78 T                   1 ~ GRB 150925A: Swift-XRT refined Analysis. MASELLI A., MELANDRI A., SBARUFATTI B., et al.
2015GCN.18368....1S 78 T                   1 ~ GRB 150925A: Swift-BAT refined analysis. SAKAMOTO T., BARTHELMY S.D., CUMMINGS J.R., et al.
2015GCN.18369....1S 78 T                   1 ~ GRB 150925A: Swift/UVOT Upper Limits. SIEGEL M.H. and RACUSIN J.L.
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.
2017ApJ...841...89A 16       D               1 54 37 Search for gravitational waves associated with gamma-ray bursts during the first Advanced LIGO observing run and implications For the origin of GRB 150906B. ABBOTT B.P., ABBOTT R., ABBOTT T.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.
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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