{"paper":{"title":"Average radio spectral energy distribution of highly star-forming galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Eva Schinnerer, Giovanni Zamorani, Huib Intema, Ivan Delvecchio, Jacinta Delhaize, Kre\\v{s}imir Tisani\\'c, Mladen Novak, Vernesa Smol\\v{c}i\\'c","submitted_at":"2018-01-25T14:38:19Z","abstract_excerpt":"The infrared-radio correlation (IRRC) offers a way to assess star formation from radio emission. Multiple studies found the IRRC to decrease with increasing redshift. This may in part be due to the lack of knowledge about the possible radio spectral energy distributions (SEDs) of star-forming galaxies. We constrain the radio SED of a complete sample of highly star-forming galaxies ($SFR>100\\,\\mathrm{M_{\\odot}}/\\,\\mathrm{yr}$) based on the VLA-COSMOS $1.4\\,\\mathrm{GHz}$ Joint and $3\\,\\mathrm{GHz}$ Large Project catalogs. We reduce archival GMRT $325\\,\\mathrm{MHz}$ and $610\\,\\mathrm{MHz}$ observ"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1801.08423","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"}