{"paper":{"title":"The host galaxies of X-ray selected Active Galactic Nuclei to z=2.5: Structure, star-formation and their relationships from CANDELS and Herschel/PACS","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Bell, A. Dekel, A. M. Koekemoer, A. Mortlock, A. Pillepich, A. Straughn, A. van der Wel, B. Magnelli, C. J. Conselice, C. J. Papovich, C. Lani, C. McPartland, C. Tonini, C. Villforth, D. C. Koo, D. Croton, D. D. Kocevski, D. H. McIntosh, D. J. Rosario, D. Lutz, D. M. Alexander, D. Snyder, E. Cheung, E. F. Bell, E. McGrath, E. O'Leary, F. Bournaud, F. E. Bauer, G. Poole, H. C. Ferguson, J. Donley, J. Guedes, J. Herrington, J. Kartaltepe, J. M. Lotz, J. R. Mullaney, J. R. Trump, K. Lai, L. DeGroot, L. J. Tacconi, M. Bernyk, M. Hilton, M. Martig, M. Mozena, M. Peth, M. Rafelski, N. A. Grogin, N. Hathi, O. Telford, P. Cassata, P. Lang, P. Popesso, P. Santini, P. Wandro, R. Bassett, R. Genzel, R. Maiolino, S. Avadhuta, S. Berta, S. M. Faber, S. Mutch, S. Wuyts, W. N. Brandt","submitted_at":"2014-09-17T20:00:02Z","abstract_excerpt":"We study the relationship between the structure and star-formation rate (SFR) of X-ray selected low and moderate luminosity active galactic nuclei (AGNs) in the two Chandra Deep Fields, using Hubble Space Telescope imaging from the Cosmic Assembly Near Infrared Extragalactic Legacy Survey (CANDELS) and deep far-infrared maps from the PEP+GOODS-Herschel survey. We derive detailed distributions of structural parameters and FIR luminosities from carefully constructed control samples of galaxies, which we then compare to those of the AGNs. At z~1, AGNs show slightly diskier light profiles than mas"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1409.5122","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"}