[ACM2000] 3-35 A , the SIMBAD biblio

We present the results of ISO observations with the CAM LW3 filter, centered at λ_eff=14.3µm, of 94 out of the 98 galaxies comprising the complete 60µm IRAS deep survey (IDS) sample in the north ecliptic polar region. In addition, we observed a source detected by IRAS at 25µm and found to have particularly interesting properties. Altogether, 106 sources were detected with a signal to noise ratio ≥3 and 69 with S/N≥5 in the 3.2'x3.2' fields centered on the nominal positions of IRAS sources. Sixty-five ≥3σ detections (49 of which at ≥5σ) are likely identifications of IRAS sources. Ten additional IRAS sources have possible ≥3σ ISOCAM counterparts. In 6 further cases, signals at the 2-3σ level were detected close to the IRAS position. Indications that IRAS sources might actually be multiple (source confusion) were found in 4 IDS fields. On the whole, we confirm the reality of 69 to 90% of IDS sources. Appropriate statistical corrections for the bias affecting faint flux estimates were applied to ISOCAM data. Ten serendipitous sources were detected at ≥5σ, with S(14.3µm)≥3.5mJy. The corresponding areal density is consistent with that found in previous surveys. Finding charts for all observed fields are given.