GRB 100807A , the SIMBAD biblio

GRB 100807A , the SIMBAD biblio (26 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST09:03:00

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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
2010GCN.11067....1G 75 T                   1 ~ GRB 100807A: Swift detection of a burst. GRUPE D., BAUMGARTNER W.H., GELBORD J.M., et al.
2010GCN.11068....1R 75 T                   1 ~ GRB 100807A: ROTSE-III optical limits. RUJOPAKARN W., FLEWELLING H., SCHAEFER B.E., et al.
2010GCN.11069....1C 75 T                   1 ~ GRB 100807A: Swift-BAT refined analysis. CUMMINGS J.R., BARTHELMY S.D., BAUMGARTNER W.H., et al.
2010GCN.11070....1O 75 T                   1 ~ GRB 100807A: enhanced Swift-XRT position. OSBORNE J.P., BEARDMORE A.P., EVANS P.A., et al.
2010GCN.11072....1S 75 T                   1 ~ GRB 100807A: Swift/UVOT upper limits. SWENSON C.A. and GRUPE D.
2010GCN.11073....1C 75 T                   1 ~ GRB 100807A: P60 optical afterglow discovery. CENKO S.B.
2010GCN.11074....1G 75 T                   1 ~ GRB 100807A: Swift XRT refined analysis. GRUPE D.
2010GCN.11075....1K 75 T                   1 ~ GRB100807A: Mitsume optical upper limits. KURODA D., YANAGISAWA K., SHIMIZU Y., et al.
2010GCN.11078....1R 75 T                   2 ~ GRB100807A: optical observation in CrAO. RUMYANTSEV V. and POZANENKO A.
2010GCN.11080....1C 75 T                   1 ~ GRB 100807A: P200 infrared observations. CHARY R. and DAVIES J.
2010GCN.11147....1K 75 T                   1 ~ GRB100807A: r band observations. KELEMEN J.
2010GCNR..295....1G 377 T         X         9 2 0 Swift Observations of
GRB 100807A. 		GRUPE D., KRIMM H.A., CUMMINGS J.R., et al.
2013MNRAS.428..729M viz 15       D               1 437 137 The prompt-afterglow connection in gamma-ray bursts: a comprehensive statistical analysis of Swift X-ray light curves. MARGUTTI R., ZANINONI E., BERNARDINI M.G., 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.
2014ApJ...787...90G viz 15       D               1 484 27 Uncovering the intrinsic variability of gamma-ray bursts. GOLKHOU V.Z. and BUTLER N.R.
2014ApJ...788...30S viz 15       D               1 328 10 Gamma-ray burst flares: X-ray flaring. II. SWENSON C.A. and ROMING P.W.A.
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.
2016ApJS..224...20Y viz 16       D               1 204 69 Comprehensive study of the X-ray flares from gamma-ray bursts observed by Swift. YI S.-X., XI S.-Q., YU H., et al.
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.
2019ApJ...884...59L viz 16       D               1 215 ~ GRB X-ray flare properties among different GRB subclasses. LIU C. and MAO J.
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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