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The large aperture GRB observatory

dc.rights.licensehttp://creativecommons.org/licenses/by-nc-sa/3.0/ve/
dc.contributor.authorAllard, D.
dc.contributor.authorAlvarez, C.
dc.contributor.authorAsorey, H.
dc.contributor.authorBarros, Humberto J. V.
dc.contributor.authorBertou, Xavier
dc.contributor.authorCastillo, M.
dc.contributor.authorChirinos, J. M.
dc.contributor.authorDe Castro, A.
dc.contributor.authorFlores, S.
dc.contributor.authorGonzález, J.
dc.contributor.authorGomez Berisso, M.
dc.contributor.authorGrajales, J.
dc.contributor.authorGuada B., Carlos E.
dc.contributor.authorW.R. Guevara, Day
dc.contributor.authorIshitsuka, J.
dc.contributor.authorLópez, J. A.
dc.contributor.authorMartínez, O.
dc.contributor.authorMelfo, A.
dc.contributor.authorMeza, E.
dc.contributor.authorMiranda Loza, P.
dc.contributor.authorMoreno Barbosa, E.
dc.contributor.authorMurrugarra, C.
dc.contributor.authorNúñez, Luis
dc.contributor.authorOtiniano Ormachea, L.J.
dc.contributor.authorPérez, G.
dc.contributor.authorPérez, Y.
dc.contributor.authorPonce, E.
dc.contributor.authorQuispe, J.
dc.contributor.authorQuintero, Carlos
dc.contributor.authorRivera, H.
dc.contributor.authorRosales R., Misael D.
dc.contributor.authorRovero, A.C.
dc.contributor.authorSaavedra, O.
dc.contributor.authorSalazare, H.
dc.contributor.authorTello, J. C.
dc.contributor.authorTicona Peraldam, R.
dc.contributor.authorVarela, E.
dc.contributor.authorVelarde, A.
dc.contributor.authorVillasenor, L.
dc.contributor.authorWahl, D.
dc.contributor.authorZamalloa, M.A.
dc.date.accessioned2010-03-19T14:27:08Z
dc.date.available2010-03-19T14:27:08Z
dc.date.issued2009-06-04
dc.identifier.urihttp://www.saber.ula.ve/handle/123456789/30672
dc.description.abstractThe Large Aperture GRB Observatory (LAGO) is aiming at the detection of the high energy (around 100GeV) component of Gamma Ray Bursts, using the single particle technique in arrays of Water Cherenkov Detectors (WCD) in high mountain sites (Chacaltaya, Bolivia, 5300m a.s.l., Pico Espejo, Venezuela, 4750m a.s.l., Sierra Negra, Mexico, 4650m a.s.l). WCD at high altitude offer a unique possibility of detecting low gamma fluxes in the 10GeV - 1TeV range. The status of the Observatory and data collected from 2007 to date will be presented.es_VE
dc.language.isoenes_VE
dc.publisherhttp://arxiv.org/es_VE
dc.rightsinfo:eu-repo/semantics/openAccess
dc.titleThe large aperture GRB observatoryes_VE
dc.typeinfo:eu-repo/semantics/article
dc.description.colacion1-4es_VE
dc.description.emailjgonzale@ula.vees_VE
dc.description.emailnunez@ula.vees_VE
dc.publisher.paisPoloniaes_VE
dc.subject.keywordsWater cherenkov detectores_VE
dc.subject.keywordsSingle particle techniquees_VE
dc.subject.keywordsGamma Ray Burstes_VE
dc.subject.tipoArtículoses_VE
dc.type.mediaTextoes_VE


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