((f)) Weak NIII{lambda}4634-40-42 emission, strong HeII{lambda}4686 absorption (f) Medium NIII{lambda}4634-40-42 emission, neutral or weak HeII{lambda}4686 absorption f Strong NIII{lambda}4634-40-42 emission, HeII{lambda}4686 emission above continuum ((f*)) NIV{lambda}4058 emission >= NIII{lambda}4640 emission, strong HeII{lambda}4686 absorption (O2-3.5) (f*) NIV{lambda}4058 emission >= NIII{lambda}4640 emission, weaker HeII{lambda}4686 absorption (O2-3.5) f* NIV{lambda}4058 emission >= NIII{lambda}4640 emission, HeII{lambda}4686 emission (O2-3.5) ((fc)) As ((f)) plus CIII{lambda}4647-50-51 emission equal to NIII{lambda}4634 (fc) As (f) plus CIII{lambda}4647-50-51 emission equal to NIII{lambda}4634 fc As f plus CIII{lambda}4647-50-51 emission equal to NIII{lambda}4634 f?p Variable CIII{lambda}4647-50-51 emission >= NIII{lambda}4634-40-42 at maximum; variable sharp absorption, emission, and/or P Cygni features at H and HeI lines ((f+)) As ((f)) plus SiIV{lambda}4089-4116 emission (O4-8, obsolete, see Section 3.1.3 of Paper I) (f+) As (f) plus SiIV{lambda}4089-4116 emission (O4-8, obsolete, see Section 3.1.3 of Paper I) f+ As f plus SiIV{lambda}4089-4116 emission (O4-8, obsolete, see Section 3.1.3 of Paper I) (e) Probable H{alpha} emission but no red spectrogram available e Emission components in H lines pe As e with emission components in HeI and/or continuum veiling [e] Emission spectrum including Fe forbidden lines e+ Fe II and H emission lines (subcategories in Lesh 1968ApJS...17..371L) ((n)) Broadened lines (not applied here, marginal) (n) More broadened lines (vsini~200km/s) n Even more broadened lines (vsini~300km/s) nn Yet even more broadened lines (vsini~400km/s) [n] H lines more broadened than He lines nfp HeII centrally reversed emission, broadened absorption lines (Conti Oef) N N absorption enhanced, C and O deficient Nstr Moderate case of above (e.g., NIII{lambda}4640 enhanced but not > CIII{lambda}4650) C C absorption enhanced, N deficient Nwk Moderate case of above var Variation in line spectrum intensities or content p Peculiar spectrum z HeII{lambda}4686 in absorption and > than both HeI{lambda}4471 and He II{lambda}4542