{"paper":{"title":"The Gould's Belt Very Large Array Survey I: The Ophiuchus complex","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Amy J. Mioduszewski, Andrew F. Boden, Cesar Brice\\~no, Gerardo Pech, Gisela N. Ortiz-Le\\'on, John Tobin, Juana L. Rivera, Laurent Loinard, Lee Hartmann, Luis F. Rodr\\'iguez, Neal J. Evans II, Rosa M. Torres, Sergio A. Dzib","submitted_at":"2013-07-19T00:30:40Z","abstract_excerpt":"We present large-scale ($\\sim$ 2000 square arcminutes), deep ($\\sim$ 20 $\\mu$Jy), high-resolution ($\\sim$ 1$''$) radio observations of the Ophiuchus star-forming complex obtained with the Karl G.\\ Jansky Very Large Array at $\\lambda$ = 4 and 6 cm. In total, 189 sources were detected, 56 of them associated with known young stellar sources, and 4 with known extragalactic objects; the other 129 remain unclassified, but most of them are most probably background quasars. The vast majority of the young stars detected at radio wavelengths have spectral types K or M, although we also detect 4 objects "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1307.5105","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"}