eUDS, SRG/eROSITA X-ray Survey of UKIDSS UDS

The resulting eROSITA UDS (or eUDS) survey was thus the first eROSITA X-ray imaging survey, which demonstrated the capability of the telescope to perform uniform observations of large sky areas. With a moderate single-camera exposure of 150ks, eUDS covered ~5deg^2^ with the limiting flux ranging between 4*10^-15^ and 5*10^-14^erg/cm^2^/s in the 0.3-2.3keV band.

We present a catalogue of 647 sources detected at likelihood >10 (~4sigma) during the eUDS. The catalogue provides information on the source fluxes in the main energy band 0.3-2.3keV and forced photometry in a number of bands between 0.3 and 8keV. Using the deeper 4XMM-DR12 catalogue, we have identified 22 strongly variable objects that have brightened or faded by at least a factor of ten during the eROSITA observations compared to previous observations by XMM-Newton.