  We evaluate the performance of the Multi-conjugate Adaptive optics
Demonstrator (MAD) from H and Ks imaging of 30 Doradus in the Large Magellanic
Cloud. Maps of the full-width half maximum (FWHM) of point sources in the H and
Ks images are presented, together with maps of the Strehl ratio achieved in the
Ks-band observations. Each of the three natural guide stars was at the edge of
the MAD field-of-view, and the observations were obtained at relatively large
airmass (1.4-1.6). Even so, the Strehl ratio achieved in the second pointing
(best-placed compared to the reference stars) ranged from 15% to an impressive
30%. Preliminary photometric calibration of the first pointing indicates 5
sigma sensitivities of Ks=21.75 and H=22.25 (from 22 and 12 min exposures,
respectively).
