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Prompt and Follow-up Multi-wavelength Observations of the GRB 161017A

AuthorsSadovnichy, V. A.; Panasyuk, M. I.; Svertilov, S. I.; Lipunov, V. M.; Bogomolov, V. V.; Gorbovskoy, E. S.; Bogomolov, A. V.; Castro-Tirado, Alberto J. ; Gabovich, A.; Hu, Y.; Iyudin, A. F.; Jeong, H. M.; Jeong, S.; Kim, M. B.; Kornilov, V. G.; Myagkova, I. N.; Park, I. H.; Petrov, V. L.; Rebolo, R.; Sánchez Ramírez, Rubén ; Reglero, V.; Sokolov, V. V.; Tyurina, N. V.; Valeev, A. F.; Vlasenko, D.; Yashin, I. V.; Yurkov, V. V.; Zhang, B. B.
KeywordsGamma-ray burst: general
Issue Date2018
PublisherIOP Publishing
CitationAstrophysical Journal 861(1): 48 (2018)
AbstractThis paper presents data on the simultaneous and complementary observations of the gamma-ray burst (GRB) GRB 161017A for optical, X-ray, and gamma wavelengths obtained by the Russian multi-messenger Lomonosov space observatory and supplemented by additional data from the Swift satellite as well as the ground-based MASTER Global Robotic Net and the 10 m Gran Telescopio Canarias. Multifrequency spectra of this very powerful explosion indicate that it originated at a distance of 10 billion light years from Earth. Here, we present the results of the prompt, early, and afterglow optical observations. The light curves and spectra suggest that the prompt optical and high-energy emissions occur in the same region near the GRB source. © 2018. The American Astronomical Society. All rights reserved.
Publisher version (URL)http://dx.doi.org/10.3847/1538-4357/aac08e
Identifiersdoi: 10.3847/1538-4357/aac08e
issn: 1538-4357
Appears in Collections:(IAA) Artículos
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