{"paper":{"title":"Polarization studies of Rotating Radio Transients","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Jameson, A. Rogers, B. W. Stappers, C.D. Ilie, C. Flynn, E.D. Barr, E. F. Keane, E. Petroff, M. Bailes, M. Caleb, P. Weltevrede, V. Venkatraman Krishnan, W. van Straten","submitted_at":"2019-05-08T14:18:08Z","abstract_excerpt":"We study the polarization properties of 22 known rotating radio transients (RRATs) with the 64-m Parkes radio telescope and present the Faraday rotation measures (RMs) for the 17 with linearly polarized flux exceeding the off-pulse noise by 3$\\sigma$. Each RM was estimated using a brute-force search over trial RMs that spanned the maximum measurable range $\\pm1.18 \\times 10^5 \\, \\mathrm{rad \\, m^2}$ (in steps of 1 $\\mathrm{rad \\, m^2}$), followed by an iterative refinement algorithm. The measured RRAT RMs are in the range |RM| $\\sim 1$ to $\\sim 950$ rad m$^{-2}$ with an average linear polariza"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1905.03080","kind":"arxiv","version":2},"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"}