  We present photometric follow-up observations of the supernova candidate AT
2018we, which was discovered by the Gaia photometric alerts system. The first
Gaia detection of the object was made Feb 12, 2018. Our observations, made in
Cousins R and Johnson B band, range from Feb 20 to May 5, 2018. From our
observations, we have constructed a light curve, which supports the initial
prediction of type Ia, included in the Gaia alert. Based on this
classification, we have also estimated the distance to its assumed host galaxy,
which was found to be around 43 Mpc.
