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