4 Conferences false [["minutes", "Minutes"], ["1", "More information about the venue"], ["notes", "Notes"], ["paper", "Paper"], ["poster", "Poster"], ["slides", "Slides"], ["summary", "Summary"]] ICN-UNAM 1482bc95ee34f0461176da21871284c8 3 icrc2007@icrc2007.unam.mx The 30th International Cosmic Ray Conference will be held from July 3, 2007 to July 11, 2007 in Merida, Yucatan, Mexico. True Merida, Mexico

2007-07-03T08:00:00 2007-07-11T19:00:00 2005-09-26T05:04:53 2024-04-12T17:46:55 Mexico/General IGeof-UNAM 40af9343b8bb9d18708b4f0252d5f53c 464 false [["minutes", "Minutes"], ["1", "More information about the venue"], ["notes", "Notes"], ["paper", "Paper"], ["poster", "Poster"], ["slides", "Slides"], ["summary", "Summary"]] OG.2.4 0 Oral Landessternwarte, ZAH, University of Heidelberg, Germany ac8929eddb28792a33ad0c97228ce6cc Landessternwarte, ZAH, University of Heidelberg, Germany ac8929eddb28792a33ad0c97228ce6cc Max-Planck-Institut fuer Kernphysik, Heidelberg, Germany d41d8cd98f00b204e9800998ecf8427e Department of Physics, University of Durham, UK d41d8cd98f00b204e9800998ecf8427e Max-Planck-Institut fuer Kernphysik, Heidelberg, Germany d41d8cd98f00b204e9800998ecf8427e Max-Planck-Institut fuer Kernphysik, Heidelberg, Germany d41d8cd98f00b204e9800998ecf8427e Landessternwarte, ZAH, University of Heidelberg, Germany d41d8cd98f00b204e9800998ecf8427e Landessternwarte, ZAH, University of Heidelberg, Germany d41d8cd98f00b204e9800998ecf8427e Merida, Mexico

Uxmal + Tulum (Holiday Inn) 2007-07-09T12:17:00 2007-07-09T12:29:00 00:12 On June 2, 2006, the Swift Burst Alert Telescope (BAT) triggered a bursting event in the 15-350 keV energy band which lasted ~9 sec. The burst position was being observed with the H.E.S.S. array of four Imaging Atmospheric Cherenkov Telescopes (IACTs) at energies above 100 GeV throughout the duration of the burst, and both before and after the burst. A total of ~5 hours of observation was obtained during that night. This is the first simultaneous observation of a soft gamma-ray bursting event with an IACT instrument. The Swift X-ray Telescope detected an X-ray counterpart starting from 83 sec after the BAT trigger. No optical/infrared counterpart was found. Due to the very soft BAT spectrum of the burst compared to other Swift gamma-ray bursts (GRBs) and its proximity to the galactic center, the burst might have been caused by a galactic X-ray burster (e.g. a low-mass X-ray binary), although the possibility of it being a cosmological GRB cannot be ruled out. We will discuss the implications of the observational data according to different bursting scenarios. paper doc http://indico.nucleares.unam.mx/images/word.png word file ppt http://indico.nucleares.unam.mx/images/powerpoint.png powerpoint file pdf http://indico.nucleares.unam.mx/images/pdf_small.png pdf file odt http://indico.nucleares.unam.mx/images/writer.png writer file odp http://indico.nucleares.unam.mx/images/impress.png presentation file ods http://indico.nucleares.unam.mx/images/calc.png spreadsheet file other http://indico.nucleares.unam.mx/images/file_small.png unknown type file link http://indico.nucleares.unam.mx/images/link.png link 1 http://www.icrc2007.unam.mx/ link http://www.icrc2007.unam.mx/ doc http://indico.nucleares.unam.mx/images/word.png word file ppt http://indico.nucleares.unam.mx/images/powerpoint.png powerpoint file pdf http://indico.nucleares.unam.mx/images/pdf_small.png pdf file odt http://indico.nucleares.unam.mx/images/writer.png writer file odp http://indico.nucleares.unam.mx/images/impress.png presentation file ods http://indico.nucleares.unam.mx/images/calc.png spreadsheet file other http://indico.nucleares.unam.mx/images/file_small.png unknown type file link http://indico.nucleares.unam.mx/images/link.png link