MOSCA is the last of our instruments to be included in the sequencer system. This will make it possible to organize and execute the observations with this instrument at the same level of flexibility as the rest of the instruments.
A new post-processing quick-look procedure was implemented that merge the images from the different CCDs while mimicking the true physical gaps between the CCDs as much as possible. A corresponding ``telescope offset'' tool was made that allows to mark any object on the combined mosaic image and move it to a desired position.