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We present near-infrared, H-band (1.65 um), surface photometry of 174 spiral galaxies in the area of the Pisces-Perseus supercluster. The images, acquired with the ARNICA camera mounted on various telescopes, are used to derive radial profiles of surface brightness, ellipticities, and position angles, together with global parameters such as H-band magnitudes and diameters. The mean relation between H-band isophotal diameter D_21.5 and the B-band D_25 implies a B-H color of the outer disk bluerdoi:10.1051/aas:1999481 fatcat:ns65766nmvfjppeapbswad52te