and flux from the literature. Col. 8: reference.

Fig. 4 shows the comparison between the E.W. (a) and flux (b) measurements reported in this paper and those found in the literature for the common objects. Fluxes and E.W. from KK83, KBS84 and GBK91 have been multiplied by 1.16, as suggested by KTC94, in order to account for the continuum flux overestimate due to the inclusion of the telluric absorption band near 6900 $\rm \AA$ in the side-band filter.

Comments to Individual Objects
------------------------------

97073: Fig. 3a reports the SPM net frame.

97093: there is a severe disagreement for this galaxy between the present measurement and the value found by MWI88 in their objective prism survey of A1367. There are no apparent reasons to suspect that our data, which were obtained under photometric sky conditions, are bad. Moreover, two early type galaxies (97088 and 97094) in the frame of 97093 (the redshift of 97094 do not match the on-band filter) result, as expected, in a null net $\rm H\alpha$ flux. However, a measured U-B = -0.31 is consistent with the MWI88 $\rm H\alpha$ value.

97129: stray light from a nearby bright star contaminates the frame.

98078: this galaxy, companion to 98081, 