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We present the results of ISO observations with the CAM LW3 lter, centered at e =1 4:3m, of 94 out of the 98 galaxies comprising the complete 60 mI RAS deep survey (IDS) sample in the north ecliptic polar re- gion. In addition, we observed a source detected by IRAS at 25m and found to have particularly interesting prop- erties. Altogether, 106 sources were detected with a signal to noise ratio 3 and 69 with S=N 5i n the 3:2 0 3:2 0 elds centered on the nominal positions of IRAS sources. Sixty-ve 3 detections (49 of which at 5) are likely identications of IRAS sources. Ten additional IRAS sources have possible 3 ISOCAM counterparts. In 6 further cases, signals at the 2 3 level were detected close to the IRAS position. Indications that IRAS sources might actually be multiple (source confusion) were found in 4 IDS elds. On the whole, we conrm the reality of 69 to 90% of IDS sources. Appropriate statistical corrections for the bias aecting faint flux estimates were applied to ISOCAM data. Ten serendipitous sources were detected at 5, with S(14:3 m) 3:5 mJy. The correspond- ing areal density is consistent with that found in previous surveys. Finding charts for all observed elds are given.

ISOCAM observations of the very deep IRAS 60 micron sample in the NEP region