  We present a sub-arcsecond cross-match of Gaia Data Release 3 (DR3) against
the INT Galactic Plane Surveys (IGAPS) and the United Kingdom Infrared Deep Sky
Survey (UKIDSS). The resulting cross-match of Galactic Plane Surveys (XGAPS)
provides additional precise photometry ($U_{RGO}$, $g$, $r$, $i$, H$\alpha$,
$J$, $H$ and $K$) to the Gaia photometry. In building the catalogue, proper
motions given in Gaia DR3 are wound back to match the epochs of the IGAPS
constituent surveys (INT Photometric \ha Survey of the Northern Galactic Plane,
IPHAS, and the UV-Excess Survey of the northern Galactic plane, UVEX) and
UKIDSS, ensuring high proper motion objects are appropriately cross-matched.
The catalogue contains 33,987,180 sources. The requirement of $>3\sigma$
parallax detection for every included source means that distances out to 1--1.5
kpc are well covered. In producing XGAPS we have also trained a Random Forest
classifier to discern targets with problematic astrometric solutions. Selection
cuts based on the classifier results can be used to clean colour-magnitude and
colour-colour diagrams in a controlled and justified manner, as well as
producing subsets of astrometrically reliable targets. We provide XGAPS as a
111 column table. Uses of the catalogue include the selection of Galactic
targets for multi-object spectroscopic surveys as well as identification of
specific Galactic populations.
