{"paper":{"title":"The GOODS-N Jansky VLA 10 GHz Pilot Survey: Sizes of Star-Forming $\\mu$Jy Radio Sources","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Andrew R. Taylor, Benjamin J. Weiner, Emmanuel Momjian, Eric J. Murphy, Hanae Inami, James J. Condon, Mark Dickinson, Ranga-Ram Chary","submitted_at":"2017-02-22T19:00:11Z","abstract_excerpt":"(Abridged) Our sensitive ($\\sigma_{\\rm n} = 572\\,{\\rm nJy\\,beam}^{-1}$), high-resolution (FWHM $\\theta_{1/2} = 220\\,{\\rm mas} \\approx2\\mathrm{\\,kpc~at~}z\\gtrsim1$) 10$\\,$GHz image covering a single Karl G.~Jansky Very Large Array (VLA) primary beam (FWHM $\\Theta_{1/2} = 4.25'$) in the GOODS-N field contains 32 sources with $S_{\\rm p}\\gtrsim2\\,\\mu{\\rm Jy~beam}^{-1}$ and optical and/or near-infrared (OIR) counterparts. Most are about as large as the star-forming regions that power them. Their median FWHM major axis is $\\langle\\theta_{\\rm M} \\rangle=167\\pm32\\,{\\rm mas} \\approx 1.2\\pm0.28\\,{\\rm kp"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1702.06963","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"}