Table B.1
References with their corresponding number of sources that contribute to our collected literature catalog.
* Using the source list from Paper I. Updated classifications for three candidate to confirmed LBVs (Sarkisyan et al. 2022; Sholukhova et al. 2020), and 11 WR stars (Neugent & Massey 2023). Removed two sources found as duplicates (original IDs: M31-957 and M31-982). Added WRs from Neugent & Massey (2023).
Notes. See notes in Appendix B.
** Using IDs from Paper I.
1 Spectral types are from Comerón et al. (2003a), while corrected coordinates from Comerón et al. (2003b).
2 Updated entries with the most recent V magnitudes for 40 BSGs from Bresolin et al. (2005).
3 Updated the list of sources presented in Schild et al. (2003), by adding 10 more sources and removing 2 (as non-WR).
4 Updated spectral types for sources initially in Roth et al. (2018) (these entries were removed from the corresponding list).
5 Two sources (stars 4 and 12) were removed as they provided broader classifications rather than the classification provided by the older work of Britavskiy et al. (2019).
6 Some V magnitudes retrieved from Massey et al. (2007b).
7 IDs OB 10-3 and UIT 136 refer to the same object. We kept the latest classification from that paper.
8 Some V magnitudes retrieved from Massey et al. (2016).
9 Confirmed LBV candidate from Massey et al. (2016).
10 Updated an uncertain YSG from Massey et al. (2016) to a RSG.
11 V-band photometry from Peña et al. (2007). HII regions 41 − 49 are knots or clumps in extended HII regions, so they were excluded from the comparison.
12 Magnitude derived from Solovyeva et al. (2019).
13 Assigned WR to all sources but kept the original classification within "[]". A magnitude value for the HeII λ4685 filter is provided wherever available; elsewhere a flag value of -99.0 is assigned.
14 Removed WR64 as duplicate to WR44, but WR35 and WR37 were kept as different (separation at 0.999″).
15 Removed all "not WR" objects (20), but kept "WN?" and "WC?" sources as WR candidates.
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