XGAPS: a sub-arcsec cross-match of galactic plane surveys

We present a sub-arcsec 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 H alpha 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 33987180 sources. The requirement of >3 sigma parallax detection for every included source means that distances out to 1-1.5kpc 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.

Automated summary

This paper presents a sub-arcsec cross-match of Gaia DR3 with IGAPS and UKIDSS, resulting in a catalogue called XGAPS. The XGAPS catalogue provides additional precise photometry to Gaia photometry and has various applications, such as selecting Galactic targets for spectroscopic surveys and identifying specific Galactic populations.