2026-06-27T23:49:55Zhttps://docta.ucm.es/rest/oai/request

oai:docta.ucm.es:20.500.14352/439332024-09-06T16:33:32Zcom_20.500.14352_14col_20.500.14352_15

00925njm 22002777a 4500 dc Antoranz Canales, Pedro author Barrio Uña, Juan Abel author Contreras González, José Luis author Fonseca González, María Victoria author Miranda Pantoja, José Miguel author Nieto Castaño, Daniel author 2010-02-10 The 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. 0004-637X 10.1088/0004-637X/710/1/828 https://hdl.handle.net/20.500.14352/43933 http://dx.doi.org/10.1088/0004-637X/710/1/828 http://iopscience.iop.org Search for very high energy gamma-ray emission from pulsar-pulsar wind nebula systems with the Magic telescope