  The coalescence of two compact objects is a key target for the new
gravitational wave observatories such as Advanced-Virgo (AdV), Advanced-LIGO
(aLIGO) and KAGRA. This phenomenon can lead to the simultaneous detection of
electromagnetic waves in the form of short GRBs (sGRBs) and gravitational wave
transients. This will potentially allow for the first time access to the
fireball and the central engine properties. We present an estimation of the
detection rate of such events, seen both by a Swift-like satellite and
AdV/ALIGO. This rate is derived only from the observations of sGRBs. We show
that this rate, if not very high, predicts a few triggers during the whole life
time of Advanced LIGO-Virgo. We discuss how to increase it using some dedicated
observational strategies. We apply our results to other missions such as the
SVOM French-Chinese satellite project or LOFT.
