{"paper":{"title":"HerMES: Spectral Energy Distributions of Submillimeter Galaxies at z >4","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Cooray, A. Efstathiou, A. J. Smith, D. Burgarella, D. Farrah, D.L. Clements, D. Riechers, D. Rigopoulou, G. G. Fazio, G. Magdis, I. Roseboom, J. Glenn, J.J. Bock, J.-S. Huang, L. Wang, M. Page, M. Rowan-Robinson, M. Symeonidis, M. Yun, S. Chapman, S. Oliver, T. M. A. Webb, Y. Dai","submitted_at":"2014-01-23T18:16:35Z","abstract_excerpt":"We present a study of the infrared properties for a sample of seven spectroscopically confirmed submillimeter galaxies at $z>$4.0. By combining ground-based near-infrared, Spitzer IRAC and MIPS, Herschel SPIRE, and ground-based submillimeter/millimeter photometry, we construct their Spectral Energy Distributions (SED) and a composite model to fit the SEDs. The model includes a stellar emission component at $\\lambda_{\\rm rest} <$ 3.5$ \\mu$m; a hot dust component peaking at $\\lambda_{rest} \\sim$ 5$\\,\\mu$m; and cold dust component which becomes significant for $\\lambda_{\\rm rest} >$ 50$\\,\\mu$m. S"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1401.6079","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"}