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The Deep Extragalactic VIsible Legacy Survey (DEVILS) is an ongoinghigh-completeness, deep spectroscopic survey of $\sim$60,000 galaxies toY$<$21.2 mag, over $\sim$6 deg2 in three well-studied deep extragalacticfields: D10 (COSMOS), D02 (XMM-LSS) and D03 (ECDFS). Numerous DEVILS projectsall require consistent, uniformly-derived and state-of-the-art photometric datawith which to measure galaxy properties. Existing photometric catalogues inthese regions either use varied photometric measurement techniques fordifferent facilities/wavelengths leading to inconsistencies, older imaging dataand/or rely on source detection and photometry techniques with known problems.Here we use the ProFound image analysis package and state-of-the-art imagingdatasets (including Subaru-HSC, VST-VOICE, VISTA-VIDEO and UltraVISTA-DR4) toderive matched-source photometry in 22 bands from the FUV to 500{\mu}m. Thisphotometry is found to be consistent, or better, in colour-analysis to previousapproaches using fixed-size apertures (which are specifically tuned to derivecolours), but produces superior total source photometry, essential for thederivation of stellar masses, star-formation rates, star-formation histories,etc. Our photometric catalogue is described in detail and, after internalDEVILS team projects, will be publicly released for use by the broaderscientific community.

Deep Extragalactic VIsible Legacy Survey (DEVILS): Consistent multi-wavelength photometry for the DEVILS regions (COSMOS, XMMLSS & ECDFS)