  We present a new speckle camera designed and built at Observatoire
Midi-Pyr\'{e}n\'{e}es. This focal instrument has been used for four years with
the 2-meter Bernard Lyot Telescope of Pic du Midi observatory. It can be set in
various operating modes: full pupil imaging, masked-pupil imaging,
spectroscopy, wave-front sensor and stellar coronagraphy, hence its name
"PISCO" ("Pupil Interferometry Speckle COronagraph"). Restored images of double
and triple stars have demonstrated its capabilities in providing close to
diffraction limited images (0.06 arcsec in V). PISCO has been fully tested and
is now ready to be used by the whole astronomical community.
