All Tables
- Table 1:
Results of the stability analysis on the INT data extension
of the selected MDM microlensing candidates. For each MDM light curve (T and C stand
respectively for Target, where we use the same numeration used in Paper I,
and Control) for which we find an astrometrically compatible INT bump, we report
the number of standard deviation within which the position and
the bump parameters (duration and flux deviation in both bands
as calculated from independent Paczynski fits on each of the MDM and INT light curves),
of the two variations are compatible.
- Table 2:
Main characteristics of the three selected short-event light curves; d is the projected distance from the centre of M 31.