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: http://www.sao.ru/precise/Laboratory/Publications/1997/CasePR/node6.html
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In this section we present the results of the spectra processing. We divided the presentation of the observed galaxies into the two main groups. In Tables 2 and 3 we give some general parameters, line intensities and equivalent widths for 142 galaxies with the detected emission lines. We summarize data in Table 4 for the rest 44 galaxies where we have not detected emission lines (in the blue part of the spectrum). One Case object CG 273 appeared to be a distant QSO. Its parameters are described separately after the main data. We present in Fig. 1 the spectra of seven emission-line galaxies and that of the quasar CG 273, in order to illustrate the main activity types in our sample.