GRB 190114C in the nuclear region of an interacting galaxy A detailed host analysis using ALMA, the HST, and the VLT
Yazar
Tanvir, N. R.
de Ugarte Postigo, A.
Thone, C. C.
Martin, S.
Japelj, J.
Levan, A. J.
Michalowski, M. J.
Selsing, J.
Kann, D. A.
Schulze, S.
Palmerio, J. T.
Vergani, S. D.
De Pasquale, M.
Bensch, K.
Covino, S.
D'Elia, V
Fruchter, A. S.
Fynbo, J. P. U.
Hartmann, D.
Heintz, K. E.
van der Horst, A. J.
Izzo, L.
Jakobsson, P.
Ng, K. C. Y.
Perley, D. A.
Rossi, A.
Sbarufatti, B.
Salvaterra, R.
Sanchez-Ramirez, R.
Watson, D.
Xu, D.
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Context. For the first time, very high energy emission up to the TeV range has been reported for a gamma-ray burst (GRB). It is still unclear whether the environmental properties of GRB 190114C might have contributed to the production of these very high energy photons, or if it is solely related to the released GRB emission.
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