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

A. de Ugarte PostigoDark Cosmology Centre, Niels Bohr Institute, Juliane Maries Vej 30, 2100 Copenhagen , DenmarkA. LundgrenEuropean Southern Observatory, Vitacura Casilla 19001, Santiago de Chile 19, ChileS. MartínD. Garcia-AppadooEuropean Southern Observatory, Vitacura Casilla 19001, Santiago de Chile 19, ChileI. de Gregorio MonsalvoA. PeckJoint ALMA Observatory, Alonso de Crdova 3107, Vitacura -Santiago, ChileM. J. MichałowskiScottish Universities Physics Alliance, Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, EH9 3HJ, UKC. C. ThöneS. CampanaINAF -Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate (LC), ItalyJ. GorosabelInstituto de Astrofsica de Andaluca (IAA-CSIC), Glorieta de la Astronoma s/n, 18008 Granada, SpainN. R. TanvirDepartment of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UKK. WiersemaDepartment of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UKA. J. Castro-TiradoInstituto de Astrofsica de Andaluca (IAA-CSIC), Glorieta de la Astronoma s/n, 18008 Granada, SpainS. SchulzeCentre for Astrophysics and Cosmology, Science Institute, University of Iceland, Dunhagi 5, 107 Reykjavk, IcelandC. De BreuckEuropean Southern Observatory, Karl Schwarzschild Strage 2, 85748 Garching, GermanyG. PetitpasHarvard-Smithsonian Center for Astrophysics, Submillimeter Array, 645 North A'ohoku Place, Hilo, HI 96720, USAJ. HjorthDark Cosmology Centre, Niels Bohr Institute, Juliane Maries Vej 30, 2100 Copenhagen , DenmarkP. JakobssonCentre for Astrophysics and Cosmology, Science Institute, University of Iceland, Dunhagi 5, 107 Reykjavk, IcelandS. CovinoINAF -Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate (LC), ItalyJ. P. U. FynboDark Cosmology Centre, Niels Bohr Institute, Juliane Maries Vej 30, 2100 Copenhagen , DenmarkJ. M. WintersInstitut de Radioastronomie Millimtrique (IRAM), 300 rue de la Piscine, 38406 Saint Martin d'Hres, FranceM. BremerInstitut de Radioastronomie Millimtrique (IRAM), 300 rue de la Piscine, 38406 Saint Martin d'Hres, FranceA. J. LevanDepartment of Physics, University of Warwick, Coventry, CV4 7AL, UKA. LlorenteHerschel Science Operations Centre, INSA, ESAC, Villafranca del Castillo, 50727, 28080 Madrid, SpainR. Sánchez-RamírezJ. C. TelloInstituto de Astrofsica de Andaluca (IAA-CSIC), Glorieta de la Astronoma s/n, 18008 Granada, SpainR. SalvaterraINAF/IASF Milano, via E. Bassini 15, 20133 Milano, Italy

2011en

ABI

Annotatsiya

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.

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DOI: 10.1051/0004-6361/201117848

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