Notes. The full table is included in Appendix C. A portion is shown here for guidance regarding its form and content. The full table contains around 2500 identifications of emission lines in the wavelength region 1700–10 400 Å from the STIS spectra of the Weigelt blobs recorded in March 1998 and February 1999. The identifications and laboratory wavelengths are from Kurucz database (Kurucz 2001). The laboratory wavelengths for parity forbidden lines are Ritz wavelengths derived from energy levels in the NIST Atomic Spectra Database (2006). All wavelengths are given in vacuum. The following comments are used: not in 98: the feature is not present in the 1998 observation. not in 99: the feature is not present in the 1999 observation. Lyα: Primary H Lyα pumped fluorescence transition. Lyα sec.: secondary H Lyα pumped fluorescence transition. 4p–4s: A 4p–4s transition, discussed in Sect. 5.5. rd sh: red shoulder due to extended stellar wind is noticeable out to +400 km s^-1. bl sh: blue shoulder due to extended stellar wind is noticeable out to –400 km s^-1. “?” the feature is weak and may not be a true emission line. “?id”: The identification is regarded as uncertain. “?E_u”: the upper level has an excitation energy  >10 eV, and the excitation mechanism is questionable. “?wl”: plausible identification, but the radial velocity differs from the mean, –45 km s^-1, by  >15 km s^-1.