Antoranz, P.Baixeras Divar, CarmenBalestra, S.Barrio, J. A.Becerra González, J.Bordas Coma, PolBosch i Ramon, ValentíBose, D.Camara, M.Contreras, J. L.Delgado Mendez, C.Fonseca, M. V.Miranda, J. M.Moldón Vara, Francisco JavierNieto, D.Oya, I.Paredes i Poy, Josep MariaRibó Gomis, MarcRobert, A.Zabalza de Torres, Víctor2013-10-112013-10-1120100004-637Xhttps://hdl.handle.net/2445/46865The 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.8 p.application/pdfeng(c) American Astronomical Society, 2010Astronomia de raigs gammaPúlsarsTelescopis espacialsNebulosesAstrofísicaGamma ray astronomyPulsarsSpace telescopesNebulaeAstrophysicsinfo:eu-repo/semantics/article5941962013-10-11info:eu-repo/semantics/openAccess