• 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. 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}
}

• A. U. Postigo, A. Lundgren, +24 authors R. Salvaterra
• Published 8 August 2011
• Physics
• 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 scientific operations of the Atacama Large Millimeter/submillimeter Array (ALMA). Aims. In this work we do a statistical analysis of the complete sample of mm/submm observations of GRB afterglows obtained before the beginning of scientific operations at ALMA. Methods. We present observations of 11 GRB afterglows obtained from the Atacama Pathfinder Experiment (APEX) and the SubMillimeter Array (SMA), as well as the first detection of a GRB with ALMA, still in the commissioning phase, and put them into context with a catalogue of all the observations that have been published until now in the spectral range that is covered by ALMA. Results. The catalogue of mm/submm observations collected here is the largest to date and is composed of 102 GRBs, of which 88 have afterglow observations, whereas the rest are host galaxy searches. With our programmes, we contributed with data of 11 GRBs and the discovery of 2 submm counterparts. In total, the full sample, including data from the literature, has 22 afterglow detections with redshifts ranging from 0.168 to 8.2. GRBs have been detected in mm/submm wavelengths with peak luminosities spanning 2.5 orders of magnitude, the most luminous reaching 10 33 erg s −1 Hz −1 . We observe a correlation between the X-ray brightness at 0.5 days and the mm/submm peak brightness. Finally we give a rough estimate of the distribution of peak flux densities of GRB afterglows, based on the current mm/submm sample. Conclusions. Observations in the mm/submm bands have been shown to be crucial for our understanding of the physics of GRBs, but have until now been limited by the sensitivity of the observatories. With the start of the operations at ALMA, the sensitivity has improved by more than an order of magnitude, opening a new era in the study of GRB afterglows and their host galaxies. Our estimates predict that, once completed, ALMA will detect up to ∼98% of the afterglows if observed during the passage of the peak synchrotron emission.