{"paper":{"title":"The Inner Debris Structure in the Fomalhaut Planetary System","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"2), (2) ASIAA, (3) NTHU, (4) CfA, (5) University of Amsterdam), Chin-Fei Lee (2) ((1) University of Arizona, David J. Wilner (4), Denis Defrere (1), George H. Rieke (1), Kate Y. L. Su (1, Kuo-Song Wang (2), Rik van Lieshout (5), Shih-Ping Lai (3","submitted_at":"2015-12-11T06:23:34Z","abstract_excerpt":"Fomalhaut plays an important role in the study of debris disks and small bodies in other planetary systems. The proximity and luminosity of the star make key features of its debris, like the water ice-line, accessible. Here we present ALMA cycle 1, 870 \\mu m (345 GHz) observations targeted at the inner part of the Fomalhaut system with a synthesized beam of 0.45\"x0.37\" (~3 AU linear resolution at the distance of Fomalhaut) and a rms of 26 \\mu Jy/beam. The high angular resolution and sensitivity of the ALMA data enable us to place strong constraints on the nature of the warm excess revealed by "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1512.03535","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"}