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Effect of local environment and stellar mass on galaxy quenching and morphology at $0.5<z<2.0$, , , , , , , , , и 13 other автор(ы). (2017)cite arxiv:1706.03780Comment: 29 pages, 15 figure, submitted to ApJ.CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey, , , , , , , , , и 96 other автор(ы). (2011)cite arxiv:1105.3753.CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey - The Hubble Space Telescope Observations, Imaging Data Products and Mosaics, , , , , , , , , и 112 other автор(ы). (2011)cite arxiv:1105.3754 Comment: 36 pages, 22 figures.Smooth(er) Stellar Mass Maps in CANDELS: Constraints on the Longevity of Clumps in High-redshift Star-forming Galaxies, , , , , , , , , и 15 other автор(ы). (2012)cite arxiv:1203.2611Comment: Submitted to The Astrophysical Journal, 25 pages, 1 table, 14 figures.A Census of Broad-Line Active Galactic Nuclei in Nearby Galaxies: Coeval Star Formation and Rapid Black Hole Growth, , , , , и . (2012)cite arxiv:1212.0544Comment: 16 pages, 17 figures. ApJ accepted.The Evolution of the Galaxy Rest-Frame Ultraviolet Luminosity Function Over the First Two Billion Years, , , , , , , , , и 19 other автор(ы). (2014)cite arxiv:1410.5439Comment: Submitted to the Astrophysical Journal. 33 pages, 20 figures, 7 tables.Confirmation of Small Dynamical and Stellar Masses for Extreme Emission Line Galaxies at z~2, , , , , , , , , и 14 other автор(ы). (2013)cite arxiv:1310.6358Comment: Accepted for publication in ApJL, 5 pages, 1 table, 4 figures.CANDELS: Constraining the AGN-Merger Connection with Host Morphologies at z~2, , , , , , , , , и 28 other автор(ы). (2011)cite arxiv:1109.2588 Comment: 10 Pages, 5 Figures, Revised draft submitted to ApJ.An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: Source catalogue and properties, , , , , , , , , и 19 other автор(ы). (2019)cite arxiv:1903.02602Comment: Submitted to MNRAS; Comments welcome. Full catalogue will be made publicly available on acceptance of paper.CEERS Key Paper III: The Resolved Host Properties of AGN at 3 < z < 5 with JWST, , , , , , , , , и 49 other автор(ы). (2022)cite arxiv:2208.14480Comment: Submitted to ApJ; 12 Pages, 6 Figures.