Notes for individual objects: 1) TX Col, an IP, which are notorious and bright X-ray emitters. X-ray source in HEAO, Swift, 1RXS. Secure CV identification 2) AH Men: this NL CV is listed as H, RXS, Swift source. Secure CV identification 3) J1015+0333: the NWAY ctp is faint, at same positional offset as the CV, not labeled as extra-galactic. The implied high f_X/f_opt excludes a coronal emitter as X-ray source. Implied optical/X-ray properties typical of a DN. Contribution by background AGN not completely excluded but unlikely. 4) 2XMM J1312: Vogel et al. (2008) identified the eclipsing polar as counterpart to the X-ray source. They also presented a spectrum of the AGN chosen by NWAY as the likely counterpart, but the periodic modulation of the X-ray signal by 100% excludes any significant contribution of the AGN to the measured X-ray signal. 5) CD-36 8436: It is an optically bright SySts, the positional offset of our proposed optical counterpart is rather large. The X-ray position is confirmed from the living Swift/XRT catalog. Both NWAY and the HamStars code (Freund et al. 2024) select a positionally better matching Gaia object as likely counterpart, a stellar coronal emitter. A possible or even likely CV mismatch. 6) ZTF19abdsnjm: The chosen counterpart by NWAY is brighter (but still implying a high X-ray to optical flux ratio), at larger positional offset, and flagged as extragalactic. While the implied the optical and X-ray properties are reasonable for a CV identification, a contribution from a background AGN cannot be excluded.