{"paper":{"title":"An SMA Continuum Survey of Circumstellar Disks in the Serpens Star-Forming Region","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"Charles J. Law, Chunhua Qi, David J. Wilner, Luca Ricci, Sean M. Andrews","submitted_at":"2017-11-03T18:00:00Z","abstract_excerpt":"We present observations with the Submillimeter Array of the continuum emission at $\\lambda = 1.3$ mm from 62 young stars surrounded by a protoplanetary disk in the Serpens star-forming region. The typical angular resolution for the survey in terms of beam size is $3.5^{\\prime \\prime}\\times2.5^{\\prime \\prime}$ with a median rms noise level of 1.6 mJy beam$^{-1}$. These data are used to infer the dust content in disks around low-mass stars $(0.1$-$2.5\\,M_{\\odot})$ at a median stellar age of $1$-$3$ Myr. Thirteen sources were detected in the 1.3 mm dust continuum with inferred dust masses of ${\\a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.01266","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"}