{"paper":{"title":"Discovery of {\\delta} Scuti Pulsations in the Young Hybrid Debris Disk Star HD 156623","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Blaine B. D. Lomberg, Eric E. Mamajek, Geert Jan J. Talens, John I. Bailey III, Konstanze Zwintz, Matthew A. Kenworthy, Michael J. Ireland, Olivier Burggraaff, Patrick Dorval, Remko Stuik, Rudi B. Kuhn, Samuel N. Mellon, Steven M. Crawford, Trevor J. David","submitted_at":"2018-11-09T19:50:39Z","abstract_excerpt":"The bRing robotic observatory network was built to search for circumplanetary material within the transiting Hill sphere of the exoplanet $\\beta$ Pic b across its bright host star $\\beta$ Pic. During the bRing survey of $\\beta$ Pic, it simultaneously monitored the brightnesses of thousands of bright stars in the southern sky ($V$ $\\simeq$ 4-8, $\\delta$ $\\lesssim$ -30$^{\\circ}$). In this work, we announce the discovery of $\\delta$ Scuti pulsations in the A-type star HD 156623 using bRing data. HD 156623 is notable as it is a well-studied young star with a dusty and gas-rich debris disk, previou"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1811.04118","kind":"arxiv","version":3},"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"}