{"paper":{"title":"The Discovery of Gas-Rich, Dusty Starbursts in Luminous Reddened Quasars at $z\\sim2.5$ with ALMA","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"C. Feruglio, C. L. Carilli, G. Jones, J. Wagg, Manda Banerji (IoA/KICC Cambridge), P. C. Hewett, R. G. McMahon, S. Alaghband-Zadeh","submitted_at":"2016-10-16T20:00:01Z","abstract_excerpt":"We present ALMA observations of cold dust and molecular gas in four high-luminosity, heavily reddened (A$_{\\rm{V}} \\sim 2.5-6$ mag) Type 1 quasars at $z\\sim2.5$ with virial M$_{\\rm{BH}} \\sim 10^{10}$M$_\\odot$, to test whether dusty, massive quasars represent the evolutionary link between submillimetre bright galaxies (SMGs) and unobscured quasars. All four quasars are detected in both the dust continuum and in the $^{12}$CO(3-2) line. The mean dust mass is 6$\\times$10$^{8}$M$_\\odot$ assuming a typical high redshift quasar spectral energy distribution (T=41K, $\\beta$=1.95 or T=47K, $\\beta$=1.6)"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.04907","kind":"arxiv","version":2},"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"}