“…Furthermore, the results reflect that the New JF-DO, comparatively, differs more markedly than do the deviate observers considered, as appears to have been deduced in a previous work. 23 However, in terms of its trend, that DO observer is more similar to the CIE-1989 SDO than to the Poza-SDO, although, as stated earlier, color observation for each observer (CIE-1989 SDO, Poza-SDO, and JF-DO) is different.…”