The observing window for Gaia17bpi has returned and we have started to look at the source again. This is the FU-Ori outbursting star we are following for the past two years now. As no fast changes are expected, we aim (like last year) to observe it in each of the filters about once a week to follow it’s progress. We only do have reliable V, R, I data, as the object is too faint for observations in B for most of our participants.
