Table A.2.
Cname, spectrum used for the measurements, extremes of the [SII] doublet calculated by the tool, and FWZI for the spectra classified as “bad” using our tool.
| Cname | MANYSPEC.Nspec | [SII]6717min | [SII]6717max | [SII]6731min | [SII]6731max | FWZI(Hα) |
|---|---|---|---|---|---|---|
| 06414719+0922535 | C20111216-00001-st.44 | – | – | – | – | 2.30 |
| 06402778+0925193 | C20120111-00001-st.118 | – | – | – | – | 2.35 |
| 06402492+0911195 | C20121205-00012-st.102 | – | – | – | – | 2.95 |
| 06392623+0947066 | C20121024-00039-st.115 | – | – | – | – | 2.60 |
| 06394446+0956006 | C20121025-00049-st.121 | – | – | – | – | 1.45 |
Notes. The complete version of this table is available at the CDS, and includes the extremes of the [NII] doublet and the object name. The FELs extremes have been derived by the sky-subtracted spectra, while the FWZI(Hα) values by the non-skysubtracted spectra. Here the information of the first five objects are reported as an example. “–” indicates flagged spurious absorption features.
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