{"paper":{"title":"VALES: II. The physical conditions of interstellar gas in normal star-forming galaxies up to z=0.2 revealed by ALMA","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Cooray, C. Furlanetto, E. Ibar, E. Valiante, E. van Kampen, L. Dunne, M. A. Lara-L\\'opez, M. Aravena, M. Baes, M. J. Micha{\\l}owski, M. W. L. Smith, N. Bourne, P. van der Werf, R. Herrera-Camus, R. J. Ivison, S. Dye, S. Eales, S. J. Maddox, T. M. Hughes, V. Villanueva, Y. Q. Xue","submitted_at":"2016-11-17T21:00:00Z","abstract_excerpt":"We use new Band-3 CO(1-0) observations taken with the Atacama Large Millimeter/submillimeter Array (ALMA) to study the physical conditions in the interstellar gas of a sample of 27 dusty main-sequence star-forming galaxies at 0.03<$z$<0.2 present in the Valpara\\'iso ALMA Line Emission Survey (VALES). The sample is drawn from far-IR bright galaxies over $\\sim$160 deg$^{2}$ in the Herschel Astrophysical Terahertz Large Area Survey (HATLAS), which is covered by Herschel [CII] 158 $\\mu$m spectroscopy and far-infrared (FIR) photometry. The [CII] and CO lines are both detected at >5$\\sigma$ in 26 so"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1611.05867","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"}