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Search for very high energy gamma-ray emission from pulsar-pulsar wind nebula systems with the MAGIC telescope

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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.

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Articles publicats en revistes (Física Quàntica i Astrofísica)

# metadata.dc.title[].value
Search for very high energy gamma-ray emission from pulsar-pulsar wind nebula systems with the MAGIC telescope