{"paper":{"title":"Radio-flaring Ultracool Dwarf Population Synthesis","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM","physics.comp-ph","physics.data-an"],"primary_cat":"astro-ph.SR","authors_text":"Matthew Route (Pennsylvania State University, Northrop Grumman Electronic Systems, Purdue University)","submitted_at":"2017-07-07T15:02:52Z","abstract_excerpt":"Over a dozen ultracool dwarfs (UCDs), low-mass objects of spectral types $\\geq$M7, are known to be sources of radio flares. These typically several-minutes-long radio bursts can be up to 100\\% circularly polarized and have high brightness temperatures, consistent with coherent emission via the electron cyclotron maser operating in $\\sim$kG magnetic fields. Recently, the statistical properties of the bulk physical parameters that describe these UCDs have become adequately described to permit synthesis of the population of radio-flaring objects. For the first time, I construct a Monte Carlo simu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1707.02212","kind":"arxiv","version":3},"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"}