Recent results from the Milagro TeV gamma-ray observatory

dc.creatorParkinson, P. M. Saz
dc.date2005-05-16
dc.date.accessioned2026-07-07T02:17:38Z
dc.date.available2026-07-07T02:17:38Z
dc.descriptionMilagro is a gamma-ray observatory employing a water Cherenkov detector to observe extensive air showers produced by high-energy particles impacting in the Earth's atmosphere. We discuss the first detection of TeV gamma-rays from the Galactic plane and report the detection of an extended TeV source coincident with the EGRET source 3EG J0520+2556, and the observation of TeV emission from the Cygnus region of our Galaxy. We also summarize the status of our search for Very High Energy (VHE) emission from satellite-triggered Gamma Ray Bursts (GRBs) and discuss plans for the next generation water Cherenkov detector.
dc.descriptionTalk presented at the "Rencontres de Moriond: Very High Energy Phenomena in the Universe" at La Thuile, Italy (March 12-19, 2005), http://moriond.in2p3.fr/J05/. To appear in the conference proceedings
dc.identifierhttps://arxiv.org/abs/astro-ph/0505335
dc.identifierhttp://arxiv.org/abs/astro-ph/0505335
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9241
dc.subjectAstrophysics
dc.titleRecent results from the Milagro TeV gamma-ray observatory
dc.typetext

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