{"paper":{"title":"The KMOS^3D Survey: Demographics and Properties of Galactic Outflows at z = 0.6 - 2.7","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Beifiori, A. Burkert, A. Renzini, A. Sternberg, C. M. Carollo, D. Lutz, D. Wilman, E. J. Nelson, E. Wisnioski, F. Eisenhauer, G. Brammer, H. \\\"Ubler, I. Momcheva, J. T. Mendel, L. J. Tacconi, M. Fabricius, M. Fossati, N. M. F\\\"orster Schreiber, P. van Dokkum, R. Genzel, R. Herrera-Camus, R. I. Davies, R. L. Davies, R. Saglia, S. Belli, S. J. Lilly, S. Price, S. Wuyts, T. Naab, T. Shimizu","submitted_at":"2018-07-12T17:42:57Z","abstract_excerpt":"We present a census of ionized gas outflows in 599 normal galaxies at redshift 0.6<z<2.7, mostly based on integral field spectroscopy of Ha, [NII], and [SII] line emission. The sample fairly homogeneously covers the main sequence of star-forming galaxies with masses 9.0<log(M*/Msun)<11.7, and probes into the regimes of quiescent galaxies and starburst outliers. About 1/3 exhibits the high-velocity component indicative of outflows, roughly equally split into winds driven by star formation (SF) and active galactic nuclei (AGN). The incidence of SF-driven winds correlates mainly with star formati"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1807.04738","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"}