GRB 140114A , the SIMBAD biblio

GRB 140114A , the SIMBAD biblio (49 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST11:34:15


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Title First 3 Authors
2014GCN.15728....1T 79 T                   1 ~ GRB 140114A: Swift detection of a burst. TROJA E., BEARDMORE A.P., BERNARDINI M.G., et al.
2014GCN.15729....1C 79 T                   1 ~ GRB 140114A: P60 observations. CENKO S.B.
2014GCN.15732....1B 79 T                   1 ~ GRB 140114A: RATIR optical and NIR afterglow detection. BUTLER N., WATSON A.M., KUTYREV A., et al.
2014GCN.15733....1B 79 T                   1 ~ GRB 140114A: enhanced Swift-XRT position. BEARDMORE A.P., EVANS P.A., GOAD M.R., et al.
2014GCN.15736....1Z 79 T                   1 ~ GRB 140114A: KAIT optical upper limit. ZHENG W., FILIPPENKO A.V., MORGAN A., et al.
2014GCN.15737....1D 79 T                   1 ~ GRB 140114A: Swift/UVOT upper limits. DE PASQUALE M. and TROJA E.
2014GCN.15738....1K 79 T                   1 ~ GRB 140114A: Swift-BAT refined analysis. KRIMM H.A., BARTHELMY S.D., BAUMGARTNER W.H., et al.
2014GCN.15739....1M 79 T                   1 ~ GRB 140114A: Swift-XRT refined analysis. MANGANO V., STROH M.C., EVANS P.A., et al.
2014GCN.15740....1G 79 T                   1 ~ GRB 140114A: ROTSE-III optical limits. GUVER T., FERRANTE F.V., KEHOE R., et al.
2014GCN.15741....1K 79 T                   1 ~ GRB 140114A: Mitsume okayama upper limits. KURODA D., YANAGISAWA K., SHIMIZU Y., et al.
2014GCN.15742....1B 79 T                   1 ~ GRB 140114A: continued RATIR optical and NIR observations. BUTLER N., WATSON A.M., KUTYREV A., et al.
2014GCN.15743....1C 79 T                   1 ~ GRB 140114A: NOT afterglow observations. CANO Z., XU D., MALESANI D., et al.
2014GCN.15756....1V 79 T                   3 ~ GRB 140114A: optical upper limit. VOLNOVA A., INASARIDZE R., KRUGLY Yu., et al.
2014ApJ...787...66Z viz 16       D               1 345 103 How long does a burst burst? ZHANG B.-B., ZHANG B., MURASE K., et al.
2015ApJ...800...16B viz 16       D               1 216 29 Are ultra-long gamma-ray bursts different? BOER M., GENDRE B. and STRATTA G.
2015MNRAS.449.2919L 135       D     X         4 39 10 A detailed study of the optical attenuation of gamma-ray bursts in the Swift era. LITTLEJOHNS O.M., BUTLER N.R., CUCCHIARA A., et al.
2015ApJ...809...76G 16       D               1 44 41 Gamma-ray bursts trace UV metrics of star formation over 3 > z ∼ 5. GREINER J., FOX D.B., SCHADY P., et al.
2015A&A...581A.125K viz 175       D     X         5 112 163 GRB hosts through cosmic time. VLT/X-Shooter emission-line spectroscopy of 96 γ-ray-burst-selected galaxies at 0.1 < z < 3.6. KRUEHLER T., MALESANI D., FYNBO J.P.U., et al.
2016MNRAS.455.4479N 16       D               1 91 10 The rapid decay phase of the afterglow as the signature of the Blandford-Znajek mechanism. NATHANAIL A., STRANTZALIS A. and CONTOPOULOS I.
2016ApJS..224...20Y viz 16       D               2 204 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.
2016ApJS..227....7L viz 16       D               1 409 56 A comparative study of long and short GRBs. I. Overlapping properties. LI Y., ZHANG B. and LU H.-J.
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.
2018ApJ...852...53R viz 16       D               1 347 27 Early X-ray flares in GRBs. RUFFINI R., WANG Y., AIMURATOV Y., et al.
2018MNRAS.474.2401V 99       D     X         3 82 ~ Thermal components in the early X-ray afterglows of GRBs: likely cocoon emission and constraints on the progenitors. VALAN V., LARSSON J. and AHLGREN B.
2018PASP..130e4202Z 16       D               1 283 2 Spectrum-energy correlations in GRBs: update, reliability, and the Long/Short dichotomy. ZHANG Z.B., ZHANG C.T., ZHAO Y.X., et al.
2018MNRAS.473.1512A viz 181       D     X         5 154 5 The Arcminute Microkelvin Imager catalogue of gamma-ray burst afterglows at 15.7 GHz. ANDERSON G.E., STALEY T.D., VAN DER HORST A.J., et al.
2018ApJ...866...97B viz 16       D               1 630 1 Statistical study of the Swift X-ray flash and X-ray rich Gamma-ray bursts. BI X., MAO J., LIU C., et al.
2019A&A...623A..92S 167           X   F     3 126 60 The X-shooter GRB afterglow legacy sample (XS-GRB). SELSING J., MALESANI D., GOLDONI P., et al.
2019MNRAS.486.2471G 17       D               2 22 ~ Can we quickly flag ultra-long gamma-ray bursts? GENDRE B., JOYCE Q.T., ORANGE N.B., et al.
2019ApJ...877..153Z 17       D               1 128 ~ Magnetar as central engine of Gamma-ray bursts: central engine-jet connection, wind-jet energy partition, and origin of some ultra-long bursts. ZOU L., ZHOU Z.-M., XIE L., et al.
2019ApJ...883...97Z 17       D               2 199 ~ The shallow decay segment of GRB X-ray afterglow revisited. ZHAO L., ZHANG B., GAO H., et al.
2019ApJ...884...59L viz 17       D               2 215 ~ GRB X-ray flare properties among different GRB subclasses. LIU C. and MAO J.
2019ApJS..245....1T 17       D               1 183 45 Statistical study of gamma-ray bursts with a plateau phase in the X-ray afterglow. TANG C.-H., HUANG Y.-F., GENG J.-J., et al.
2020ApJ...893...77W viz 17       D               1 3281 34 A comprehensive statistical study of gamma-ray bursts. WANG F., ZOU Y.-C., LIU F., et al.
2020ApJS..248...21H viz 17       D               1 390 ~ Revisiting the relationship between the long GRB rate and cosmic star formation history based on a large Swift sample. HAO J.-M., CAO L., LU Y.-J., et al.
2020MNRAS.494.5259Y 17       D               1 204 ~ Less noticeable shallow decay phase in early X-ray afterglows of GeV/TeV-detected gamma-ray bursts. YAMAZAKI R., SATO Y., SAKAMOTO T., et al.
2020ApJ...896L..20J viz 17       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...908...83T viz 17       D               1 173 19 The Konus-Wind Catalog of gamma-ray Bursts with known redshifts. II. Waiting-mode Bursts simultaneously detected by Swift/BAT. TSVETKOVA A., FREDERIKS D., SVINKIN D., 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.
2021MNRAS.508...52L 17       D               1 424 4 Revisiting the luminosity and redshift distributions of long gamma-ray bursts. LAN G.-X., WEI J.-J., ZENG H.-D., et al.
2021ApJ...922...34C 17       D               2 52 ~ A comprehensive study of multiflare GRB spectral lag. CHANG X.Z., PENG Z.Y., CHEN J.M., et al.
2022ApJ...924...69Y viz 18       D               1 134 10 Statistical analyses of the energies of X-ray plateaus and flares in gamma-ray bursts. YI S.-X., DU M. and LIU T.
2022ApJ...939..116A 18       D               2 61 21 Searches for Neutrinos from Gamma-Ray Bursts Using the IceCube Neutrino Observatory. ABBASI R., ACKERMANN M., ADAMS J., et al.
2023MNRAS.520.5764C 19       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.
2023ApJS..267...42D viz 19       D               1 455 ~ A Stochastic Approach to Reconstruct Gamma-Ray-burst Light Curves. DAINOTTI M.G., SHARMA R., NARENDRA A., et al.
2023MNRAS.525.3262B 19       D               1 227 ~ Understanding the nature of the optical emission in gamma-ray bursts: analysis from TAROT, COATLI, and RATIR observations. BECERRA R.L., KLOTZ A., ATTEIA J.L., et al.
2023ApJS..269....2S 19       D               1 228 ~ Statistical Analysis of Long GRBs' Prompt Emission and X-Ray Flares: Multivariate Clustering and Correlations. SAJI J., IYYANI S. and MAZDE K.

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