Notes. The table is divided into four segments. The top one includes those stars for which the analysis presented in Sect. 4 indicates that they are in all probability ssrAp stars. The spectroscopic properties of the stars listed in the second segment are consistent with their having either moderately or extremely long rotation periods. The rotation period of the star from the third segment probably is moderately long (20 d ≲ P_rot ≲ 50 d). The fourth segment contains the only magnetic Ap star of this study to have a rotation period of a few days. In each segment, the stars are listed in order of increasing TIC number (Col. 1); an alternative ID is given is Col. 2. The visible range spectrum of those stars for which ‘x’ appears in Col. 3 shows resolved magnetically split lines; the ‘x’ flag in Col. 4 identifies those stars for which a significant detection of the magnetic field was achieved and at least one field moment could be determined, either in this study or in the literature (see text). Column 5 indicates which stars are spectroscopic binaries, distinguishing to the extent possible the single-lined (SB1) and double-lined systems. Finally, in Col. 6, we list the value of the rotation period, when available from the literature (the references are given in the relevant sub-sections of Sect. 4) or an estimated value or lower limit derived as part of the present study.