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Spectral modelling of a H.E.S.S.-detected pulsar wind nebula
(SAIP, 2015)
In the last decade ground-based Imaging Atmospheric Cherenkov Telescopes have
discovered roughly 30 pulsar wind nebulae at energies above 100 GeV. We present first results
from a leptonic emission code that models the ...
High-energy emission properties of pulsars
(PoS, 2017)
The sheer number of new γ-ray pulsar discoveries by the Fermi Large Area Telescope since 2008,
combined with the quality of new multi-frequency data, has caused a revolution in the field of
high-energy rotation-powered ...