Gaia transient detection efficiency: hunting for nuclear transients
  We present a study of the detectability of transient events associated with
galaxies for the Gaia European Space Agency astrometric mission. We simulated
the on-board detections, and on-ground processing for a mock galaxy catalogue
to establish the properties required for the discovery of transient events by
Gaia, specifically tidal disruption events (TDEs) and supernovae (SNe).
Transients may either be discovered by the on-board detection of a new source
or by the brightening of a previously known source. We show that Gaia
transients can be identified as new detections on-board for offsets from the
host galaxy nucleus of 0.1--0.5,arcsec, depending on magnitude and scanning
angle. The Gaia detection system shows no significant loss of SNe at close
radial distances to the nucleus. We used the detection efficiencies to predict
the number of transients events discovered by Gaia. For a limiting magnitude of
19, we expect around 1300 SNe per year: 65% SN Ia, 28% SN II and 7% SN Ibc, and
~20 TDEs per year.
