{"paper":{"title":"On the incidence of \\textit{WISE} infrared excess among solar analog, twin and sibling stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"Ant\\^onio D. Costa, Bruno L. Canto Martins, Daniel B. de Freitas, Danielly Freire da Silva, Izan C. Le\\~ao, Jos\\'e E. Lima Jr, Jos\\'e R. De Medeiros","submitted_at":"2016-11-07T20:16:42Z","abstract_excerpt":"This study presents a search for IR excess in the 3.4, 4.6, 12 and 22 $\\mu$m bands in a sample of 216 targets, composed of solar sibling, twin and analog stars observed by the \\textit{WISE} mission. In general, an infrared excess suggests the existence of warm dust around a star. We detected 12 $\\mu$m and/or 22 $\\mu$m excesses at the 3$\\sigma$ level of confidence in five solar analog stars, corresponding to a frequency of 4.1 $\\%$ of the entire sample of solar analogs analyzed, and in one out of 29 solar sibling candidates, confirming previous studies. The estimation of the dust properties sho"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1611.02250","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"}