Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/46865
Full metadata record
DC FieldValueLanguage
dc.contributor.authorAntoranz, P.-
dc.contributor.authorBaixeras Divar, Carmen-
dc.contributor.authorBalestra, S.-
dc.contributor.authorBarrio, J. A.-
dc.contributor.authorBecerra González, J.-
dc.contributor.authorBordas Coma, Pol-
dc.contributor.authorBosch i Ramon, Valentí-
dc.contributor.authorBose, D.-
dc.contributor.authorCamara, M.-
dc.contributor.authorContreras, J. L.-
dc.contributor.authorDelgado Mendez, C.-
dc.contributor.authorFonseca, M. V.-
dc.contributor.authorMiranda, J. M.-
dc.contributor.authorMoldón Vara, Francisco Javier-
dc.contributor.authorNieto, D.-
dc.contributor.authorOya, I.-
dc.contributor.authorParedes i Poy, Josep Maria-
dc.contributor.authorRibó Gomis, Marc-
dc.contributor.authorRobert, A.-
dc.contributor.authorZabalza de Torres, Víctor-
dc.date.accessioned2013-10-11T07:56:28Z-
dc.date.available2013-10-11T07:56:28Z-
dc.date.issued2010-
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/2445/46865-
dc.description.abstractThe MAGIC collaboration has searched for high-energy gamma-ray emission of some of the most promising pulsar candidates above an energy threshold of 50 GeV, an energy not reachable up to now by other ground-based instruments. Neither pulsed nor steady gamma-ray emission has been observed at energies of 100 GeV from the classical radio pulsars PSR J0205+6449 and PSR J2229+6114 (and their nebulae 3C58 and Boomerang, respectively) and the millisecond pulsar PSR J0218+4232. Here, we present the flux upper limits for these sources and discuss their implications in the context of current model predictions.-
dc.format.extent8 p.-
dc.format.mimetypeapplication/pdf-
dc.language.isoeng-
dc.publisherInstitute of Physics (IOP)-
dc.relation.isformatofReproducció del document publicat a: http://dx.doi.org/10.1088/0004-637X/710/1/828-
dc.relation.ispartofAstrophysical Journal, 2010, vol. 710, num. 1, p. 828-835-
dc.relation.urihttp://dx.doi.org/10.1088/0004-637X/710/1/828-
dc.rights(c) American Astronomical Society, 2010-
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)-
dc.subject.classificationAstronomia de raigs gamma-
dc.subject.classificationPúlsars-
dc.subject.classificationTelescopis espacials-
dc.subject.classificationNebuloses-
dc.subject.classificationAstrofísica-
dc.subject.otherGamma ray astronomy-
dc.subject.otherPulsars-
dc.subject.otherSpace telescopes-
dc.subject.otherNebulae-
dc.subject.otherAstrophysics-
dc.titleSearch for very high energy gamma-ray emission from pulsar-pulsar wind nebula systems with the MAGIC telescope-
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.identifier.idgrec594196-
dc.date.updated2013-10-11T07:56:28Z-
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

Files in This Item:
File Description SizeFormat 
594196.pdf867 kBAdobe PDFView/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.