Back to Search Start Over

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

Authors :
Ministry of Education and Science of the Russian Federation
Ministerio de Economía y Competitividad (España)
European Commission
Lomonosov Moscow State University
National Research Foundation of Korea
Institute for Basic Science (South Korea)
Russian Foundation for Basic Research
Russian Science Foundation
Sadovnichy, 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, Vladimir V.
Tyurina, N. V.
Valeev, A. F.
Vlasenko, D.
Yashin, I. V.
Yurkov, V. V.
Zhang, B. B.
Ministry of Education and Science of the Russian Federation
Ministerio de Economía y Competitividad (España)
European Commission
Lomonosov Moscow State University
National Research Foundation of Korea
Institute for Basic Science (South Korea)
Russian Foundation for Basic Research
Russian Science Foundation
Sadovnichy, 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, Vladimir V.
Tyurina, N. V.
Valeev, A. F.
Vlasenko, D.
Yashin, I. V.
Yurkov, V. V.
Zhang, B. B.
Publication Year :
2018

Abstract

This 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.

Details

Database :
OAIster
Publication Type :
Electronic Resource
Accession number :
edsoai.on1286548929
Document Type :
Electronic Resource