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Very-high energy emission from pulsars
(SAIP, 2015)
The vast majority of pulsars detected by the Fermi Large Area Telescope (LAT)
display exponentially cutoff spectra with cutoffs falling in a narrow band around a few GeV.
Early spectral modelling predicted spectral cutoffs ...
The effect of different magnetospheric structures on predictions of gamma-ray pulsar light curves
(SAIP, 2014)
The second pulsar catalogue of the Fermi Large Area Telescope (LAT) will contain
in excess of 100 gamma-ray pulsars. The light curves (LCs) of these pulsars exhibit a variety
of shapes, and also different relative phase ...
The effect of an offset-dipole magnetic field on the Vela pulsar’s γ-ray light curves
(SAIP, 2015)
Over the past six years, the Fermi Large Area Telescope has detected more than
150 γ-ray pulsars, discovering a variety of light curve trends and classes. Such diversity hints
at distinct underlying magnetospheric and/or ...
Pulsar emission in the very-high-energy regime
(Sissa Medialab, 2015)
The vast majority of the pulsars detected by the Fermi Large Area Telescope (LAT) display spectra
with exponential cutoffs falling in a narrow range around a few GeV. Early spectral modelling
predicted spectral cutoff ...
The effect of different magnetospheric structures on predictions of gamma-ray pulsar light curves
(South African Institute of Physics, 2012)
The second pulsar catalogue of the Fermi Large Area Telescope (LAT) will contain in excess of 100 gamma-ray pulsars. The light curves (LCs) of these pulsars exhibit a variety of shapes, and also different relative phase ...