{"paper":{"title":"Satellite Quenching and Galactic Conformity at 0.3 < z < 2.5","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Adam R. Tomczak, Avishai Dekel, Caroline Straatman, Casey Papovich, Daniel D. Kelson, David C. Koo, Eric Persson, Glenn G. Kacprzak, Ivo Labb\\'e, Joel R. Primack, Karl Glazebrook, Kim-Vy Tran, Lalitwadee Kawinwanichakij, Lee R. Spitler, Michael Cowley, Peter S. Behroozi, Pieter van Dokkum, Rebecca Allen, Ryan F. Quadri, Seong-Kook Lee, Themiya Nanayakkara, Vithal Tilvi, William G. Hartley, Yu Lu","submitted_at":"2015-11-09T21:00:02Z","abstract_excerpt":"We measure the evolution of the quiescent fraction and quenching efficiency of satellites around star-forming and quiescent central galaxies with stellar mass $\\log(M_{\\mathrm{cen}}/M_{\\odot})>10.5$ at $0.3<z<2.5$. We combine imaging from three deep near-infrared-selected surveys (ZFOURGE/CANDELS, UDS, and UltraVISTA), which allows us to select a stellar-mass complete sample of satellites with $\\log(M_{\\mathrm{sat}}/M_{\\odot})>9.3$. Satellites for both star-forming and quiescent central galaxies have higher quiescent fractions compared to field galaxies matched in stellar mass at all redshifts"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1511.02862","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"}