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We present the final reduction and calibration of the FIRBACK ISOPHOT data.FIRBACK is a deep cosmological survey performed at 170 microns. This paperdeals with the ISOPHOT C200 camera with the C160 filter. We review the wholedata reduction process and compare our final calibration with DIRBE (for theextended emission) and IRAS (for point sources). The FIRBACK source extractionand galaxy counts is discussed in a companion paper (Dole et al., 2001).

FIRBACK. II. Data reduction and calibration of the 170 $\mathsf{\mu}$m ISO deep cosmological survey