Mostrar el registro sencillo del ítem

Operating water cherenkov detectors in high altitude sites for 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.authorMezal, 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.accessioned2010-03-18T22:17:10Z
dc.date.available2010-03-18T22:17:10Z
dc.date.issued2009-06-04
dc.identifier.urihttp://www.saber.ula.ve/handle/123456789/30671
dc.description.abstractWater Cherenkov Detectors (WCD) are efficient detectors for detecting GRBs in the 10 GeV - 1 TeV energy range using the single particle technique, given their sensitivity to low energy secondary photons produced by high energy photons when cascading in the atmosphere. The Large Aperture GRB Observatory (LAGO) operates arrays of WCD in high altitude sites (above 4500ma.s.l.) in Bolivia, Mexico and Venezuela, with planned extension to Peru. Details on the operation and stability of these WCD in remote sites with high background rates of particles will be detailed, and compared to simulations. Specific issues due to operation at high altitude, atmospheric effects and solar activity, as well as possible hardware enhancements will also be presented.es_VE
dc.language.isoenes_VE
dc.publisherhttp://arxiv.org/es_VE
dc.rightsinfo:eu-repo/semantics/openAccess
dc.titleOperating water cherenkov detectors in high altitude sites for the large aperture GRB observatoryes_VE
dc.typeinfo:eu-repo/semantics/article
dc.description.colacion1-5es_VE
dc.description.emailjgonzale@ula.vees_VE
dc.description.emailnunez@ula.vees_VE
dc.publisher.paisPoloniaes_VE
dc.subject.keywordsNew experimentses_VE
dc.subject.keywordsWater cherenkov detectorses_VE
dc.subject.keywordsHigh energy photonses_VE
dc.subject.tipoArtículoses_VE
dc.type.mediaTextoes_VE


Ficheros en el ítem

Thumbnail
Nombre:
09061.pdf
Tamaño:
434.3Kb
Formato:
PDF
Ver/

Este ítem aparece en la(s) siguiente(s) colección(ones)

Mostrar el registro sencillo del ítem