{"paper":{"title":"Mass assembly and morphological transformations since $z\\sim3$ from CANDELS","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Dekel, A.M. Koekemoer, C. Conselice, D.C. Koo, D.D. Kocevski, E. Daddi, F. Shankar, G. Barro, J.S. Kartaltepe, M. Bernardi, M. Huertas-Company, M.L.N. Ashby, N.A. Grogin, P. Dimauro, P.G.P\\'erez-Gonz\\'alez, S. Mei, S.M. Faber","submitted_at":"2016-06-15T20:00:08Z","abstract_excerpt":"[abridged] We quantify the evolution of the stellar mass functions of star-forming and quiescent galaxies as a function of morphology from $z\\sim 3$ to the present. Our sample consists of ~50,000 galaxies in the CANDELS fields ($\\sim880$ $arcmin^2$), which we divide into four main morphological types, i.e. pure bulge dominated systems, pure spiral disk dominated, intermediate 2-component bulge+disk systems and irregular disturbed galaxies. Our main results are:\n  Star-formation: At $z\\sim 2$, 80\\% of the stellar mass density of star-forming galaxies is in irregular systems. However, by $z\\sim "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1606.04952","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"}