{"paper":{"title":"The Bright and Dark Sides of High-Redshift starburst galaxies from {\\it Herschel} and {\\it Subaru} observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Calabr\\`o, A. Franceschini, A. Man, A. Puglisi, A. Renzini, B. Darvish, C. Maier, C. Mancini, D. B. Sanders, D. Kashino, E. Daddi, F. Valentino, G. Rodighiero, J. D. Silverman, J. S. Kartaltepe, L. Rodr\\'iguez-Mu\\~noz, S. Jin, V. Mainieri","submitted_at":"2017-03-14T22:51:55Z","abstract_excerpt":"We present rest-frame optical spectra from the FMOS-COSMOS survey of twelve $z \\sim 1.6$ \\textit{Herschel} starburst galaxies, with Star Formation Rate (SFR) elevated by $\\times$8, on average, above the star-forming Main Sequence (MS). Comparing the H$\\alpha$ to IR luminosity ratio and the Balmer Decrement we find that the optically-thin regions of the sources contain on average only $\\sim 10$ percent of the total SFR whereas $\\sim90$ percent comes from an extremely obscured component which is revealed only by far-IR observations and is optically-thick even in H$\\alpha$. We measure the [NII]$_"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1703.04801","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"}