{"paper":{"title":"Evolution of Dust-Obscured Star Formation and Gas to z=2.2 from HiZELS","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alasdair Thomson (Durham), David Sobral, Edo Ibar, Helen Johnson, Ian Smail, James Geach, James Simpson, Mark Swinbank, Philip Best","submitted_at":"2017-02-20T21:42:25Z","abstract_excerpt":"We investigate the far-infrared properties of galaxies selected via deep, narrow-band imaging of the H$\\alpha$ emission line in four redshift slices from $z=0.40$--$2.23$ over $\\sim 1$deg$^2$ as part of the High-redshift Emission Line Survey (HiZELS). We use a stacking approach in the Herschel PACS/SPIRE bands, along with $850\\,\\mu$m imaging from SCUBA-2 to study the evolution of the dust properties of H$\\alpha$-emitters selected above an evolving characteristic luminosity threshold, $0.2L^\\star_{{\\rm H}\\alpha}(z)$. We investigate the relationship between the dust temperatures and the far-infr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1702.06182","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"}