{"paper":{"title":"The emission and distribution of dust of the torus of NGC 1068","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Almudena Alonso-Herrero, Andreas Efstathiou, Attila Kovavcs, Chris Packham, Cristina Ramos Almeida, Dominic J. Benford, Doyal Harper, Enrique Lopez-Rodriguez, Fabio P. Santos, James Radomski, J. Staguhn, Kohei Ichikawa, Lindsay Fuller, Marc Berthoud, Nancy A. Levenson, Ryan Hamilton, Terry Herter","submitted_at":"2018-04-11T18:00:01Z","abstract_excerpt":"We present observations of NGC 1068 covering the $19.7-53.0$ $\\mu$m wavelength range using FORCAST and HAWC+ onboard SOFIA. Using these observations, high-angular resolution infrared (IR) and sub-mm observations, we find an observational turn-over of the torus emission in the $30-40$ $\\mu$m wavelength range with a characteristic temperature of $70-100$ K. This component is clearly different from the diffuse extended emission in the narrow line and star formation regions at 10-100 $\\mu$m within the central 700 pc. We compute $2.2-432$ $\\mu$m 2D images using the best inferred \\textsc{clumpy} tor"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1804.04134","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"}