X-shooter and ALMA spectroscopy of GRB 161023A A study of metals and molecules in the line of sight towards a luminous GRB
Author
COVINO, S.
Mundell, C. G.
Murphy, D.
Oates, S.
Salmon, L.
VAN SOELEN, B.
Tanvir, N. R.
Turpin, D.
XU, D.
ZAFAR, T.
De Pasquale, Massımılıano
DE UGARTE POSTIGO, A.
THONE, C. C.
Hansen, M.
Hartmann, D. H.
Heintz, K. E.
JAKOBSSON, P.
Kobayashi, S.
BOLMER, J.
Schulze, S.
MARTIN, S.
KANN, D. A.
D'ELIA, V.
Selsing, J.
Martin-Carrillo, A.
Perley, D. A.
KIM, S.
IZZO, L.
SANCHEZ-RAMIREZ, R.
GUIDORZI, C.
Klotz, A.
Wiersema, K.
BAUER, F. E.
BENSCH, K.
Campana, S.
CANO, Z.
COWARD, D.
DE CIA, A.
de Gregorio-Monsalvo, I.
Fynbo, J. P. U.
GREINER, J.
GOMBOC, A.
Hanlon, L.
Malesani, D. B.
MARTONE, R.
MEINTJES, P. J.
MICHALOWSKI, M. J.
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Context. Long gamma-ray bursts (GRBs) are produced during the dramatic deaths of massive stars with very short lifetimes, meaning that they explode close to the birth place of their progenitors. Over a short period they become the most luminous objects observable in the Universe, being perfect beacons to study high-redshift star-forming regions.
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