{"paper":{"title":"Is there a relationship between AGN and star formation in IR-bright AGNs?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Adam Atanas, Alain Omont, Belinda J. Wilkes, Harry I. Teplitz, Jacqueline Bergeron, Joanna Kuraszkiewicz, Y. Sophia Dai","submitted_at":"2015-11-20T20:59:59Z","abstract_excerpt":"We report the relationship between the luminosities of active galactic nuclei (AGNs) and the rates of star formation (SF) for a sample of 323 far-infrared (FIR)-detected AGNs. This sample has a redshift range of 0.2 $< z <$ 2.5, and spans three orders of magnitude in luminosity, ${\\rm L_{X} \\sim 10^{42-45}}$erg$s^{-1}$. We find that in AGN hosts, the total IR luminosity (8-1000$\\mu$m) has a significant AGN contribution (average$\\sim$20%), and we suggest using the FIR luminosity (30-1000 $\\mu$m) as a more reliable star formation rate (SFR) estimator. We also conclude that monochromatic luminosi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1511.06761","kind":"arxiv","version":5},"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"}