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Weitere Publikationen von Autoren mit dem selben Namen

Transient-optimised real-bogus classification with Bayesian Convolutional Neural Networks -- sifting the GOTO candidate stream, , , , , , , , , und 38 andere Autor(en). (2021)cite arxiv:2102.09892Comment: 17 pages, 12 figures, resubmitted to MNRAS following reviewer comments.Self-Supervised Clustering on Image-Subtracted Data with Deep-Embedded Self-Organizing Map., , , , , , , , , und 38 andere Autor(en). CoRR, (2022)GOODS-Herschel~: Gas-to-dust mass ratios and CO-to-H_2 conversion factors in normal and starbursting galaxies at high-z, , , , , , , , , und 8 andere Autor(en). (2011)cite arxiv:1109.1140 Comment: Accepted for publication in ApJ.ALMA observations of a z~3.1 Protocluster: Star Formation from Active Galactic Nuclei and Lyman-Alpha Blobs in an Overdense Environment, , , , , , , , , und 7 andere Autor(en). (2016)cite arxiv:1601.00682Comment: MNRAS, submitted: 9 pages, 3 figures, 2 tables.The hidden AGN main sequence: Evidence for a universal SMBH accretion to star formation rate ratio since z~2 producing a M_BH-M* relation, , , , , , , , und . (2012)cite arxiv:1204.2824Comment: 6 Pages, 3 Figures, Submitted to ApJL.Concurrent Supermassive Black Hole and Galaxy Growth: Linking Environment and Nuclear Activity in z = 2.23 H-alpha Emitters, , , , , , , , , und 2 andere Autor(en). (2013)cite arxiv:1301.3922Comment: 11 pages, 5 figures, accepted for publication in ApJ.The KMOS AGN Survey at High redshift (KASHz): the prevalence and drivers of ionised outflows in the host galaxies of X-ray AGN, , , , , , , , , und . (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, , , und . (12.03.2014)A remarkably flat relationship between the average star formation rate and AGN luminosity for distant X-ray AGN, , , , , , , und . (26.02.2015)ALMA and Herschel reveal that AGN and main-sequence galaxies have different star formation rate distributions, , , , , , , , , und 8 andere Autor(en). (2015)cite arxiv:1506.05459Comment: 5 pages, 3 figures, 1 table; Submitted to MNRAS.