First significant detection of gamma-ray pulsed radiation variations associated with a glitch in PSR J0205+6449, with changes in peak amplitude ratio and separation attributed to magnetospheric reconfiguration.
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2 Pith papers cite this work, alongside 28 external citations. Polarity classification is still indexing.
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TeV-selected PWNe and unidentified sources yield beaming fractions of 0.1-0.3 across radio, gamma-ray, and X-ray bands, with survey-to-survey differences explained by selection biases or older pulsars and reproducible via time-dependent opening angles.
citing papers explorer
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Discovery of Short-Term {\gamma}-Ray Pulsed Radiation Variations Following a Glitch in PSR J0205+6449
First significant detection of gamma-ray pulsed radiation variations associated with a glitch in PSR J0205+6449, with changes in peak amplitude ratio and separation attributed to magnetospheric reconfiguration.
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Constraining the Pulsar Beaming Fraction with TeV-Selected Galactic Pulsar Wind Nebulae and unidentified TeV Sources
TeV-selected PWNe and unidentified sources yield beaming fractions of 0.1-0.3 across radio, gamma-ray, and X-ray bands, with survey-to-survey differences explained by selection biases or older pulsars and reproducible via time-dependent opening angles.