Pre-ALMA observations of GRBs in the mm/submm range

A. Postigo; A. Lundgren; S. Martin; D. Garcia-Appadoo; I. D. G. Monsalvo; A. Peck; M. J. Michałowski; C. Thone; S. Campana; J. Gorosabel; N. Tanvir; K. Wiersema; A. Castro-Tirado; S. Schulze; C. D. Breuck; G.Petitpas; J. Hjorth; P. Jakobsson; S. Covino; J. Fynbo; J. Winters; M. Bremer; A. Levan; A. Llorente; R. S'anchez-Ram'irez; J. C. Tello; R. Salvaterra

DOI:10.1051/0004-6361/201117848

Corpus ID: 59140684

Pre-ALMA observations of GRBs in the mm/submm range

@article{Postigo2011PreALMAOO,
  title={Pre-ALMA observations of GRBs in the mm/submm range},
  author={A. Postigo and A. Lundgren and S. Martin and D. Garcia-Appadoo and I. D. G. Monsalvo and A. Peck and M. J. Michałowski and C. Thone and S. Campana and J. Gorosabel and N. Tanvir and K. Wiersema and A. Castro-Tirado and S. Schulze and C. D. Breuck and G.Petitpas and J. Hjorth and P. Jakobsson and S. Covino and J. Fynbo and J. Winters and M. Bremer and A. Levan and A. Llorente and R. S'anchez-Ram'irez and J. C. Tello and R. Salvaterra},
  journal={Scopus},
  year={2011}
}

A. Postigo, A. Lundgren, +24 authors R. Salvaterra

Published 2011

Physics, Computer Science

Scopus

Context. Gamma-ray bursts (GRBs) generate an afterglow emission that can be detected from radio to X-rays during days, or even weeks after the initial explosion. The peak of this emission crosses the millimeter and submillimeter range during the first hours to days, making their study in this range crucial for constraining the models. Observations have been limited until now due to the low sensitivity of the observatories in this range. This situation will be greatly improved with the start of… CONTINUE READING

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