GRB 100420A , the SIMBAD biblio

GRB 100420A , the SIMBAD biblio (26 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST19:52:38


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Title First 3 Authors
2010GCN.10628....1B 75 T                   1 ~ GRB 100420A: Swift detection of a burst. BAUMGARTNER W.H., BURROWS D.N., CHESTER M.M., et al.
2010GCN.10629....1X 75 T                   1 ~ GRB 100420A: ROTSE-III optical limits. XIAO L., RUJOPAKARN W., SCHAEFER B.E., et al.
2010GCN.10636....1U 75 T                   1 ~ GRB 100420A: SARA upper limits. UPDIKE A.C., HARTMANN D.H. and DE PREE C.
2010GCN.10638....1B 75 T                   1 ~ GRB 100420A: enhanced Swift-XRT position. BEARDMORE A.P., EVANS P.A., GOAD M.R., et al.
2010GCN.10639....1R 75 T                   1 ~ GRB 100420A: XRT refined analysis. ROWLINSON A. and BAUMGARTNER W.H.
2010GCN.10640....1C 75 T                   1 ~ GRB 100420A: Swift/UVOT upper limits. CHESTER M.M. and BAUMGARTNER W.H.
2010GCN.10642....1K 75 T                   1 ~ GRB100420A: Mitsume optical upper limits. KURODA D., YANAGISAWA K., SHIMIZU Y., et al.
2010GCN.10660....1C 75 T                   1 ~ GRB 100420A: Swift-BAT refined analysis. CUMMINGS J.R., BARTHELMY S.D., BAUMGARTNER W.H., et al.
2010GCN.10666....1S 75 T                   1 ~ GRB 100420A: GRT optical observation. SAKAMOTO T., DONATO D., GEHRELS N., et al.
2010GCN.10704....1A 75 T                   1 ~ GRB 100420A: terskol optical upper limit. ANDREEV M., SERGEEV A., VOLNOVA A., et al.
2010GCN.10706....1L 75 T                   1 ~ GRB 100420A: Gemini discovery of infrared afterglow. LEVAN A.J., CUCCHIARA A. and TANVIR N.R.
2010GCN.10707....1F 75 T                   1 ~ GRB 100420A: EVLA radio observations. FRAIL D.A. and CHANDRA P.
2012ApJ...746..156C viz 15       D               2 305 185 A radio-selected sample of gamma-ray burst afterglows. CHANDRA P. and FRAIL D.A.
2012ApJ...746..170M viz 15       D               1 355 10 Rapid, machine-learned resource allocation: application to high-redshift gamma-ray burst follow-up. MORGAN A.N., LONG J., RICHARDS J.W., et al.
2012ApJ...760...12A viz 15       D               1 159 104 Search for gravitational waves associated with gamma-ray bursts during LIGO science run 6 and Virgo science runs 2 and 3. ABADIE J., ABBOTT B.P., ABBOTT R., et al.
2013ApJS..209...20G viz 15       D               1 754 27 Evidence for new relations between gamma-ray burst prompt and X-ray afterglow emission from 9 years of Swift. GRUPE D., NOUSEK J.A., VERES P., et al.
2014ApJ...787...66Z viz 15       D               1 345 103 How long does a burst burst? ZHANG B.-B., ZHANG B., MURASE K., et al.
2015MNRAS.448.2624C viz 16       D               1 1121 5 Catalogue of isolated emission episodes in gamma-ray bursts from Fermi, Swift and BATSE. CHARISI M., MARKA S. and BARTOS I.
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.
2017MNRAS.464.4545B viz 16       D               1 924 18 Galaxy gas as obscurer - I. GRBs x-ray galaxies and find an N_ H_3∝M_*_ relation. BUCHNER J., SCHULZE S. and BAUER F.E.
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.
2021MNRAS.503.3262Z 17       D               1 333 ~ How are gamma-ray burst radio afterglows populated? ZHANG K., ZHANG Z.B., HUANG Y.F., 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.
2023MNRAS.520.5764C 17       D               1 340 2 Radio-bright versus radio-dark gamma-ray bursts - more evidence for distinct progenitors. CHAKRABORTY A., DAINOTTI M., CANTRELL O., 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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