  Since 2009 we are running a project to identify flashes produced by the
impact of meteoroids on the surface of the Moon. For this purpose we are
employing small telescopes and high-sensitivity CCD video cameras. To
automatically identify these events a software package called MIDAS was
developed and tested. This package can also perform the photometric analysis of
these flashes and estimate the value of the luminous efficiency. Besides, we
have implemented in MIDAS a new method to establish which is the likely source
of the meteoroids (known meteoroid stream or sporadic background). The main
features of this computer program are analyzed here, and some examples of lunar
impact events are presented.
