arXiv · 0908.0717
VERITAS Observations of Magnetars
Abstract
Magnetars are rotating neutron stars with extremely strong magnetic fields (~ 10^14-10^15 G). X-ray and soft gamma-ray observations have revealed the existence of non-thermal particle populations which may suggest emission of very high energy photons. VERITAS, an array of four 12m imaging atmospheric Cherenkov telescopes, is designed to observe gamma-ray emission between 100 GeV and 30 TeV. Here we present the results of VERITAS observations of two magnetars, 4U 0142+61 and 1E 2259+586.
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R. Guenette. 2009-08-05. VERITAS Observations of Magnetars. https://arxiv.org/abs/0908.0717
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