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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3 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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2026 3representative citing papers
LAMBDA proposes megameter-scale baselines using additional Australian stations to extend SKA-Low for high-resolution low-frequency VLBI.
No measurable changes in radio and X-ray emission were observed around four glitches in PSR J2229+6114, providing evidence that magnetar-like post-glitch activity is more common in high-B rotation-powered pulsars.
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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Low-frequency VLBI with the SKA-Low
LAMBDA proposes megameter-scale baselines using additional Australian stations to extend SKA-Low for high-resolution low-frequency VLBI.
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No Measurable Changes in Radio and X-ray Emission Surrounding Glitches in the Young Pulsar PSR J2229+6114
No measurable changes in radio and X-ray emission were observed around four glitches in PSR J2229+6114, providing evidence that magnetar-like post-glitch activity is more common in high-B rotation-powered pulsars.