{"paper":{"title":"Herschel-ATLAS: Correlations between Dust and Gas in Local Submm-Selected Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"A. Cooray, A. Dariush, C. J. R. Clark, D. J. B. Smith, E. E. Rigby, E. Ibar, E. Valiante, G. de Zotti, G. J. Bendo, K. Rowlands, L. Dunne, L. L. Leeuw, M. A. Thompson, M. Baes, M. J. Jarvis, M. J. Micha{\\l}owski, M. N. Bremer, M. W. L. Smith, N. Bourne, R. Hopwood, R. J. Ivison, S. Dye, S. Eales, S. J. Maddox","submitted_at":"2013-08-20T20:00:03Z","abstract_excerpt":"We present an analysis of CO molecular gas tracers in a sample of 500{\\mu}m-selected Herschel-ATLAS galaxies at z<0.05 (cz<14990km/s). Using 22-500{\\mu}m photometry from WISE, IRAS and Herschel, with HI data from the literature, we investigate correlations between warm and cold dust, and tracers of the gas in different phases. The correlation between global CO(3-2) line fluxes and FIR-submillimetre fluxes weakens with increasing IR wavelength ({\\lambda}>60{\\mu}m), as a result of colder dust being less strongly associated with dense gas. Conversely, CO(2-1) and HI line fluxes both appear to be "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1308.4406","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"}