{"paper":{"title":"A detailed study of giant pulses from PSR B1937+21 using the Large European Array for Pulsars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"B. W. Stappers, C. G. Bassa, D. Perrodin, G. H. Janssen, I. Cognard, J. W. McKee, K. J. Lee, K. Liu, L. Wang, M. Gaikwad, M. Kramer, R. Karuppusamy, R. Smits, S. A. Sanidas, S. Chen, W. W. Zhu","submitted_at":"2018-11-07T12:21:54Z","abstract_excerpt":"We have studied 4265 giant pulses (GPs) from the millisecond pulsar B1937+21; the largest-ever sample gathered for this pulsar, in observations made with the Large European Array for Pulsars. The pulse energy distribution of GPs associated with the interpulse are well-described by a power law, with index $\\alpha = -3.99 \\pm 0.04$, while those associated with the main pulse are best-described by a broken power law, with the break occurring at $\\sim7$ Jy $\\mu$s, with power law indices $\\alpha_{\\text{low}} = -3.48 \\pm 0.04$ and $\\alpha_{\\text{high}} = -2.10 \\pm 0.09$. The modulation indices of th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1811.02856","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}