Notes. This is one out of 60 tables, each corresponding to a different aperture (see Sect. 3.3). We show our selection considering a 2 kpc aperture. From the first to the last column, the table is shown as it is stored in the supplementary data. The first column reports the ID of the row. The second column reports the Plate and IFU of the corresponding target. In the third column, a boolean array is stored to flag a galaxy as an AGN if the value is 1, and not an AGN if the value is 0 (i.e., Seyferts and LINERs with EW(Hα) > 3 Å). From the fourth to the eighth column, the BPT class is shown. We abbreviate Seyferts, LINERs, star-forming, composite, and ambiguous classifications as SY, LI, SF, CM, and AM, respectively (however, in the fits table, they are tagged with their full name). From Cols. 9 to 12, the emission line flux ratios are given as logarithmic bases of 10. Lastly, the last column stores the information of the EW in Å. If a value is tagged as nan, the emission line did not pass our S/N criteria (see Sect. 3.2.)