4 candidate dusty WC identifications in IRS 13E (WR101de, 101df, 101dh, 101ea) primarily from Maillard et al. (2004, MPS04) were not supported by Fritz et al. (FGD10)
8 stars from original manuscript of Kanarek et al. (2014, KSF14). 1089-117 omitted since spectroscopy reveals MgII 2.13/2.14 micron emission so LBV candidate Stringfellow et al. (2012). 1626-4FC8 is a [WC6] according to Gvaramadze et al. (2010). Other sources also omitted 1343-69E, 1353-160A, 1430-AB0, 1443-760, 1547-1DF2, 1547-E0B, some of which are reclassified as PNe or B[e]/LBVs.
1 star from Shara et al. (2012), 1023-63L (WC7) subsequently reclassified as a CSPNe [WC7] by Kanarek et al. 2016 (KSF16).