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

@article{Postigo2011PreALMAOO,
  title={Pre-ALMA observations of GRBs in the mm/submm range},
  author={Antonio de Ugarte Postigo and Andreas Andersson Lundgren and S. Mart'in and Diego Garcia-Appadoo and I. de Gregorio Monsalvo and Alison B. Peck and Michał Jerzy Michałowski and Christina C. Thone and Sergio Campana and Javier Gorosabel and Nial R. Tanvir and Klaas Wiersema and Alberto J. Castro-Tirado and Steve Schulze and Carlos de Breuck and G.Petitpas and Jens Hjorth and P. Jakobsson and Stefano Covino and Johan P. U. Fynbo and Jack M. Winters and Michael Bremer and Andrew J. Levan and {\'A}lvaro Llorente and Rub'en S'anchez-Ram'irez and J. C. Tello and Ruben Salvaterra},
  journal={Scopus},
  year={2011}
}
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… 

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