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The KMOS AGN Survey at High redshift (KASHz): the prevalence and drivers of ionised outflows in the host galaxies of X-ray AGN

, , , , , , , , , and . (2015)cite arxiv:1511.00008Comment: Re-submmited to MNRAS after addressing referee's comments. Main paper: 20 pages, 14 figures. Plus appendix.

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The KMOS AGN Survey at High redshift (KASHz): the prevalence and drivers of ionised outflows in the host galaxies of X-ray AGN, , , , , , , , , and . (2015)cite arxiv:1511.00008Comment: Re-submmited to MNRAS after addressing referee's comments. Main paper: 20 pages, 14 figures. Plus appendix.Kiloparsec-scale outflows are prevalent among luminous AGN: outflows and feedback in the context of the overall AGN population, , , and . (Mar 12, 2014)Curves and surfaces in computer aided geometric design: Fujio Yamaguchi, Springer-Verlag (1988), 378 pp, ISBN 0-387-17449-4.. Comput. Aided Des., 24 (1): 63 (1992)Concurrent Supermassive Black Hole and Galaxy Growth: Linking Environment and Nuclear Activity in z = 2.23 H-alpha Emitters, , , , , , , , , and 2 other author(s). (2013)cite arxiv:1301.3922Comment: 11 pages, 5 figures, accepted for publication in ApJ.The KMOS Redshift One Spectroscopic Survey (KROSS): rotational velocities and angular momentum of z~0.9 galaxies, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1701.05561Comment: Re-submitted to MNRAS after addressing referee's comments. Table of values and extended figures available at: http://astro.dur.ac.uk/KROSS/.The KMOS Deep Survey (KDS) I: dynamical measurements of typical star-forming galaxies at z $\simeq$ 3.5, , , , , , , , , and . (2017)cite arxiv:1704.06263Comment: main body 25 pages, 8 figures.ALMA observations of a z~3.1 Protocluster: Star Formation from Active Galactic Nuclei and Lyman-Alpha Blobs in an Overdense Environment, , , , , , , , , and 7 other author(s). (2016)cite arxiv:1601.00682Comment: MNRAS, submitted: 9 pages, 3 figures, 2 tables.A remarkably flat relationship between the average star formation rate and AGN luminosity for distant X-ray AGN, , , , , , , and . (Feb 26, 2015)Do AGN really suppress star formation?, , , , and . (2019)cite arxiv:1912.01020Comment: IAU Proceedings No. 356 "Nuclear Activity in Galaxies Across Cosmic Time", M. Povic et al.An imperfectly passive nature: Bright sub-millimeter emission from dust-obscured star formation in the z=3.717 "passive" system, ZF20115, , , , , , , , , and 21 other author(s). (2017)cite arxiv:1704.03868Comment: ApJ submitted. Comments welcome.