Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010apj...710..828a&link_type=abstract
The Astrophysical Journal, Volume 710, Issue 1, pp. 828-835 (2010).
Astronomy and Astrophysics
Astronomy
1
Gamma Rays: Stars, Methods: Observational, Pulsars: Individual: Psr J0205+6449 Psr J2229+6114 Psr J0218+4232, Telescopes
Scientific paper
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.
Anderhub H.
Antonelli Lucio Angelo
Antoranz P.
Backes Michael
Baixeras Carmen
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