eROSITA CalPV (observation on October 11, 2019) and eRASS1 (started on April 26, 2020) light curves in the 0.2–0.8 (red) and 0.8–7 (blue) keV bands. The CalPV light curves obtained using three cameras (TM5,6,7) are normalised to seven cameras, as all seven cameras were active during the eSASS1 observation. During the eROSITA all-sky survey observations both the soft- and hard-band count rates increased. The variability in the soft and hard bands is not as dramatic as that seen in the PV observations.