The giant pulse population of PSR B0355+54

arXiv:2605.21469 · astro-ph.HE · Submitted 2026-05-20 · Read on arXiv

astro-ph.HE

Submitted: 2026-05-20

Updated: 2026-06-10

Comments: Submitted to Elsevier

Journal ref: Journal of High Energy Astrophysics, Volume 56, 2027

DOI: 10.1016/j.jheap.2026.100741

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Consistency — 3× in this paper · explained in 3 episodes
• Trace — 2× in this paper · explained in 2 episodes
• Active Regions — 1× in this paper · explained in 1 episode
• Generative AI — 1× in this paper · explained in 2 episodes
• Quantization — 1× in this paper · explained in 12 episodes

Sources

• A broadband radio study of the average profile and giant pulses from PSR B1821-24A
• Properties and Interpretations of Giant Micropulses and Giant Pulses from Pulsars
• Variability of the Pulsed Radio Emission from the Large Magellanic Cloud Pulsar PSR J0529-6652
• Is pulsar B0656+14 a very nearby RRAT source?
• The bright spiky emission of pulsar B0656+14

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