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Table 3.

Confirmed accretors with flag.

CNAME FLAG CLASS
06392550+0931394 SII II
06393398+0949208 SII
06393939+0945215 SII II
06394147+0946196 SII
06395328+0949458 SII III
06395795+0941046 SII II
06400215+0945143 SII III
06400553+0922261 SII II
06400600+0949426 SII II
06401418+0934284 SII II
06401780+0925478 SII II
06402150+0906031 SII II
06403652+0950456 SII II
06403698+0939098 SII
06403746+0955212 SII III
06403912+0950586 SII II
06404132+0951023 SII II
06404185+0951445 SII II
06404601+0917582 SII
06405059+0954573 SII
06405364+0933247 SII II
06405426+0949203 SII II
06405518+0950498 SII III
06405572+0951138 SII II
06405883+0939187 SII II
06410712+0912383 SII II
06411292+0905257 SII II
06411600+0916351 SII II
06412402+1014321 SII
06412419+0948309 SII II
06412562+0934430 SII II
06413729+0945066 SII II
06414188+0919282 SII II
06415307+0958034 SII
06415493+0942527 SII
06405295+0926256 NII II
06404940+0952540 SII OR NII II
06401111+0921272 SII AND NII
06404136+0954138 SII AND NII II

Notes. These confirmed accretors (see Venuti et al. 2018) show spurious [SII] doublet (FLAG = SII) or spurious [NII] doublet (FLAG = NII) in absorption or both (FLAG = SII AND NII, if in the same spectrum; FLAG = SII OR NII, if different spectra) in at least one spectrum, therefore are flagged by our automated tool. Their class as derived by Venuti et al. (2018) is also indicated in the last column.

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