The optical identification of events with poorly defined locations: the case of the Fermi GBM GRB 140801A

Lipunov, V.M.; Gorosabel, J.; Pruzhinskaya, M.V.; de Ugarte, P.A.; Pelassa, V.; Tsvetkova, A.E.; Sokolov, I.V.; Kann, D.A.; Dong, X.; Gorbovskoy, E.S.; Krushinski, V.V.; Kornilov, V.G.; Balanutsa, P.V.; Boronina, S.V.; Budnev, N.M.; Cano, Z.; Castro-Tirado, A.J.; Chazov, V.V.; Connaughton, V.; Delvaux, C.; Frederiks, D.D.; Fynbo, J.F.; Gabovich, A.V.; Goldstein, A.; Greiner, J.; Gress, O.A.; Ivanov, K.I.; Jakobsson, P.; Klose, S.; Knust, F.; Komarova, V.N.; Konstantinov, E.; Krylov, A.V.; Kuvshinov, D.A.; Kuznetsov, A.S.; Lipunova, G.V.; Moskvitin, A.S.; Pal'shin, V.D.; Pandey, S.B.; Poleshchuk, V.A.; Schmidl, S.; Sergienko, Y.P.; Sinyakov, E.V.; Schulze, S.; Sokolov, V.V.; Sokolova, T.N.; Sparre, M.; Thöne, C.C.; Tlatov, A.G.; Tyurina, N.V.; Ulanov, M.V.; Yazev, S.A.; Yurkov, V.V.

Авторы: Lipunov V.M., Gorosabel J., Pruzhinskaya M.V., de Ugarte Postigo A., Pelassa V., Tsvetkova A.E., Sokolov I.V., Kann D.A., Dong Xu, Gorbovskoy E.S., Krushinski V.V., Kornilov V.G., Balanutsa P.V., Boronina S.V., Budnev N.M., Cano Z., Castro-Tirado A.J., Chazov V.V., Connaughton V., Delvaux C., Frederiks D.D., Fynbo J.F.U, Gabovich A.V., Goldstein A., Greiner J., Gress O.A., Ivanov K.I., Jakobsson P., Klose S., Knust F., Komarova V.N., Konstantinov E., Krylov A.V., Kuvshinov D.A., Kuznetsov A.S., Lipunova G.V., Moskvitin A.S., Pal'shin V.D., Pandey S.B., Poleshchuk V.A., Schmidl S., Sergienko Yu P., Sinyakov E.V., Schulze S., Sokolov V.V., Sokolova T.N., Sparre M., Thöne C.C., Tlatov A.G., Tyurina N.V., Ulanov M.V., Yazev S.A., Yurkov V.V.
Журнал: Monthly Notices of the Royal Astronomical Society
Том: 455
Номер:
Год издания: 2016
Издательство: Oxford Journals, Oxford University Press
Местоположение издательства: Oxford, UK, England
Первая страница: 712
Последняя страница: 724
DOI: 10.1093/mnras/stv2228
Аннотация: We report the early discovery of the optical afterglow of gamma-ray burst (GRB) 140801A in the 137 deg2 3-σ error-box of the Fermi Gamma-ray Burst Monitor (GBM). MASTER is the only observatory that automatically reacts to all Fermi alerts. GRB 140801A is one of the few GRBs whose optical counterpart was discovered solely from its GBM localization. The optical afterglow of GRB 140801A was found by MASTER Global Robotic Net 53 s after receiving the alert, making it the fastest optical detection of a GRB from a GBM error-box. Spectroscopy obtained with the 10.4-m Gran Telescopio Canarias and the 6-m Big Telescope Alt-azimuth of the Special Astrophysical Observatory of the Russian Academy of Sciences reveals a redshift of z = 1.32. We performed optical and near-infrared photometry of GRB 140801A using different telescopes with apertures ranging from 0.4 to 10.4 m. GRB 140801A is a typical burst in many ways. The rest-frame bolometric isotropic energy release and peak energy of the burst are Eiso=5.54+0.26−0.24×1052 erg and Ep, rest ≃ 280 keV, respectively, which is consistent with the Amati relation. The absence of a jet break in the optical light curve provides a lower limit on the half-opening angle of the jet θ = 6∘.1. The observed Epeak is consistent with the limit derived from the Ghirlanda relation. The joint Fermi GBM and Konus-Wind analysis show that GRB 140801A could belong to the class of intermediate duration. The rapid detection of the optical counterpart of GRB 140801A is especially important regarding the upcoming experiments with large coordinate error-box areas.
Добавил в систему: Липунов Владимир Михайлович

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The optical identification of events with poorly defined locations: the case of the Fermi GBM GRB 140801Aстатья

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