  We present imaging results and source counts from an ISOCAM deep and
ultra-deep cosmological survey through gravitationally lensing clusters of
galaxies at 7 and 15 microns. A total area of about 53 sq.arcmin was covered in
maps of three clusters. The lensing increases the sensitivity of the survey. A
large number of luminous mid-infrared (MIR) sources were detected behind the
lenses, and most could be unambiguously identified with visible counterparts.
Thanks to the gravitational amplification, these results include the faintest
MIR detections ever recorded, extending source counts to an unprecedented
level. The source counts, corrected for cluster contamination and lensing
distortion effects, show an excess by a factor of 10 with respect to the
prediction of a no-evolution model, as we reported for A2390 alone in Altieri
et al. (1999). These results support the A2390 result that the resolved 7 and
15 microns background radiation intensities are 1.7 (+/- 0.5) x 10^-9 and 3.3
(+/- 1.3) x 10^-9 W/m^2/sr, respectively, integrating from 30 microJy to 50
mJy.
