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Observations of environmental quenching in groups in the 11 Gyr since z=2.5: different quenching for central and satellite galaxies, , , , , , , , , and 9 other author(s). (2014)cite arxiv:1401.2984Comment: Submitted to ApJ.Satellite Quenching and Galactic Conformity at 0.3 < z < 2.5, , , , , , , , , and 14 other author(s). (2015)cite arxiv:1511.02862Comment: Submitted to ApJ after first round of referee comments, 22 pages, 12 figures.Effect of local environment and stellar mass on galaxy quenching and morphology at $0.5<z<2.0$, , , , , , , , , and 13 other author(s). (2017)cite arxiv:1706.03780Comment: 29 pages, 15 figure, submitted to ApJ.The distribution of satellites around massive galaxies at 1<z<3 in ZFOURGE/CANDELS: dependence on star formation activity, , , , , , , , , and 16 other author(s). (2014)cite arxiv:1406.6056Comment: 19 pages, 17 figures, Resubmitted to ApJ after responding to referee report. Information on ZFOURGE can be found at http://zfourge.tamu.edu.Discovery of Extreme OIII+H$\beta$ Emitting Galaxies Tracing an Overdensity at z~3.5 in CDF-South, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1703.03814Comment: Accepted for publication in ApJL. 8 pages, 4 figures.Exploring the z=3-4 massive galaxy population with ZFOURGE: the prevalence of dusty and quiescent galaxies, , , , , , , , , and 10 other author(s). (2014)cite arxiv:1405.1048Comment: Accepted for publication in ApJ Letters. See http://zfourge.tamu.edu for more details about ZFOURGE.Galaxy Stellar Mass Functions from ZFOURGE/CANDELS: An Excess of Low-Mass Galaxies Since z=2 and the Rapid Buildup of Quiescent Galaxies, , , , , , , , , and 8 other author(s). (2013)cite arxiv:1309.5972Comment: 12 pages, 11 figures. Submitted for publication in the ApJ.Tracing the Star Formation-Density Relation to z~2, , , and . (2011)cite arxiv:1104.1426 Comment: Submitted to ApJ. 14 pages, including appendix.The number density and mass density of star-forming and quiescent galaxies at 0.4 &lt; z &lt; 2.2, , , , , , , , , and 2 other author(s). (2011)cite arxiv:1104.2595 Comment: Submitted to the Astrophysical Journal. The release of EAZY v2.0 will accompany the publication of the manuscript in the journal.