This tool provides a forecast of times targets cross the Gaia Focal Plane.
It is based on the scanning operations of Gaia. It does not take into account operational activities preventing nominal observations nor matters like e.g.
the gaps between CCDs on the Focal Plane.
Adding up all dead time components, users should understand that the probability of the data of the target being received on the ground at the indicated time is about 80%.
Furthermore, only targets in magnitude range 6<G<20 mag are observed in astrometry and photometry and 6<G_RVS<16 mag in spectroscopy.
Please note that one more spin phase adjustment to the Gaia orbit will be implemented at a later stage.
Therefore the predicted observation time may deviate by up to 6 hours from the actual observation time.