{"paper":{"title":"Continuum sources from the THOR survey between 1 and 2 GHz","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM","astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"A. Brunthaler, A.J. Walsh, F. Bigiel, H. Beuther, H. Linz, J.M. Stil, J. Ott, J.S. Urquhart, K.G. Johnston, K.M. Menten, L.D. Anderson, M.H. Heyer, M. Rugel, N.M. McClure-Griffiths, R. Plume, R. Shanahan, R.S. Klessen, S. Bihr, S.C.O. Glover, S.N. Longmore, T. Henning, T. Schierhuber","submitted_at":"2016-01-13T22:18:01Z","abstract_excerpt":"We carried out a large program with the Karl G. Jansky Very Large Array (VLA): \"THOR: The HI, OH, Recombination line survey of the Milky Way\". We observed a significant portion of the Galactic plane in the first quadrant of the Milky Way in the 21cm HI line, 4 OH transitions, 19 radio recombination lines, and continuum from 1 to 2 GHz. In this paper we present a catalog of the continuum sources in the first half of the survey (l=14.0-37.9deg and l=47.1-51.2deg, |b|<1.1deg) at a spatial resolution of 10-25\", with a spatially varying noise level of ~0.3-1 mJy/beam. The catalog contains ~4400 sou"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1601.03427","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"}