{"paper":{"title":"The AGN Luminosity Fraction in Merging Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"2), (2) University of Arizona Astronomy Department, 3), (3) Rensselaer Polytechnic Institute Department of Physics, (4) Flatiron Institute Center for Computational Astrophysics, 5), (5) Leiden Observatory, (6) California Institute of Technology Department of Astronomy, 7, (7) University of Crete Physics Department & Institute of Theoretical Computational Physics, 8) ((1) Harvard-Smithsonian Center for Astrophysics, (8) Foundation for Research, Aaron S. Weiner (1, Andreas Zezas (1, Andr\\'es F. Ramos Padilla (1, Applied Physics, Astronomy, AZ, CA, Cambridge, Christopher C. Hayward (4), Crete, Greece, Greece), Heraklion, Howard A. Smith (1), Jeremy Dietrich (1, Juan Rafael Mart\\'inez-Galarza (1), Lee Rosenthal (6), Leiden, MA, Matthew L.N. Ashby (1), Netherlands, New York, NY, Pasadena, S.P. Willner (1), Steward Observatory, Technology-Hellas, Troy, Tucson","submitted_at":"2018-01-12T21:51:17Z","abstract_excerpt":"Galaxy mergers are key events in galaxy evolution, often causing massive starbursts and fueling active galactic nuclei (AGN). In these highly dynamic systems, it is not yet precisely known how much starbursts and AGN respectively contribute to the total luminosity, at what interaction stages they occur, and how long they persist. Here we estimate the fraction of the bolometric infrared (IR) luminosity that can be attributed to AGN by measuring and modeling the full ultraviolet to far-infrared spectral energy distributions (SEDs) in up to 33 broad bands for 24 merging galaxies with the Code for"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1801.04328","kind":"arxiv","version":2},"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"}