{"paper":{"title":"CO Spectral Line Energy Distributions of IR-luminous galaxies and AGN","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Emmanuel M. Xilouris, Kate Isaak, Padeli P. Papadopoulos, Paul van der Werf","submitted_at":"2010-03-30T18:31:11Z","abstract_excerpt":"We  report on  new sensitive  CO J=6-5  line observations  of several luminous  infrared Galaxies  (LIRGs: L$_{\\rm  IR}$(8-1000$\\mu $m$)\\ga 10^{11}$ L$_{\\odot}$),   36%  (8/22)   of  them   ULIRGs  (L$_{\\rm IR}$$>10^{12}$ L$_{\\odot}$),  and  two   powerful  local  AGN:  the optically  luminous QSO  PG 1119+120, and  the powerful  radio galaxy 3C 293 using the James Clerk Maxwell Telescope (JCMT) on Mauna Kea in Hawaii.  We combine these observations with existing low-J CO data and dust emission Spectral Energy Distributions (SEDs) in the far-infrared - submillimetre from the literature to cons"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1003.5889","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"}