dc.contributor.author Ramasawmy, Joanna dc.contributor.author Stevens, Jason dc.contributor.author Martin, Garreth dc.contributor.author Geach, James E. dc.date.accessioned 2019-05-23T14:05:14Z dc.date.available 2019-05-23T14:05:14Z dc.date.issued 2019-04-17 dc.identifier.citation Ramasawmy , J , Stevens , J , Martin , G & Geach , J E 2019 , ' A flat trend of star-formation rate with X-ray luminosity of galaxies hosting AGN in the SCUBA-2 Cosmology Legacy Survey ' , Monthly Notices of the Royal Astronomical Society , vol. 486 , pp. 4320-4333 . https://doi.org/10.1093/mnras/stz1093 dc.identifier.issn 0035-8711 dc.identifier.other PURE: 16663910 dc.identifier.other PURE UUID: f8c83292-1a06-4d5c-934f-21461764791f dc.identifier.other ArXiv: http://arxiv.org/abs/1904.07880v1 dc.identifier.uri http://hdl.handle.net/2299/21348 dc.description © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. dc.description.abstract Feedback processes from active galactic nuclei (AGN) are thought to play a crucial role in regulating star formation in massive galaxies. Previous studies using \textit{Herschel} have resulted in conflicting conclusions as to whether star formation is quenched, enhanced, or not affected by AGN feedback. We use new deep 850 $\mu$m observations from the SCUBA-2 Cosmology Legacy survey (S2CLS) to investigate star formation in a sample of X-ray selected AGN, probing galaxies up to $L_{0.5-7~\rm keV} = 10^{46}$ erg s$^{-1}$. Here we present the results of our analysis on a sample of 1957 galaxies at \$ 1
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