Table D.1.
Fluxes, errors, and S/Ns of detected oxygen and sulphur auroral lines for each galaxy in the sample.
| Galaxy ID | [O III]λ5007 Flux | S/N | [O II]λ3727 Flux | S/N | [S II]λ4068 Flux | S/N | [S III]λ6312 Flux | S/N |
|---|---|---|---|---|---|---|---|---|
| (×10−19) | (×10−19) | (×10−19) | (×10−19) | |||||
| MARTA_3942 | 3.51 ± 0.38 | 5.0 | 12.8 ± 0.99 | 6.4 | 3.3 ± 1.1 | 7.5 | 5.28 ± 0.67 | 5.0 |
| MARTA_4195 | 1.12 ± 0.45 | 6.3 | 6.02 ± 0.81 | 6.6 | 0.634 ± 0.12 | 3.2 | – | – |
| MARTA_5014 | 1.33 ± 0.28 | 6.3 | 11.6 ± 0.56 | 12 | – | – | – | – |
| MARTA_552 | 7.12 ± 0.26 | 22 | 4.71 ± 0.53 | 6.9 | – | – | 3.04 ± 0.58 | 3.9 |
| MARTA_2387 | 1.39 ± 0.28 | 4.2 | 2.54 ± 0.56 | 3.8 | – | – | – | – |
| MARTA_4327 | 6.54 ± 0.26 | 15 | 14.4 ± 0.50 | 12 | 3.36 ± 0.25 | 8.2 | 1.98 ± 0.39 | 5.1 |
| MARTA_4502 | 2.16 ± 0.25 | 13 | 6.80 ± 0.52 | 6.1 | 1.94 ± 0.25 | 3.8 | – | – |
| MARTA_3408 | 1.68 ± 0.36 | 4.0 | – | – | – | – | – | – |
| MARTA_414 | 2.59 ± 0.30 | 7.8 | – | – | – | – | – | – |
| MARTA_4471 | 2.07 ± 0.33 | 4.9 | – | – | – | – | – | – |
| MARTA_329 | 2.65 ± 0.63 | 4.3 | – | – | – | – | – | – |
| MARTA_1084 | 0.51 ± 0.4 | 2.6† | 2.25 ± 0.74 | 4.6 | – | – | – | – |
| MARTA_3115 | 1.50 ± 0.32 | 3.3 | – | – | – | – | – | – |
| MARTA_1374 | 3.12 ± 0.12 | 6.1 | – | – | – | – | – | – |
| MARTA_3887 | 7.43 ± 0.51 | 11 | – | – | – | – | – | – |
| MARTA_3926 | 1.10 ± 0.43 | 7.5 | – | – | – | – | – | – |
Notes. Fluxes are given in units of 10−19 erg/s/cm2, with errors on the fluxes estimated by the PPXF fitting. The S/Ns are calculated by multiplying the peak flux by 
, with N being the number of spectral channels spanned by line FWHM, and dividing it by the RMS measured in a line-free adjacent region.
( † )The S/N estimated from the PPXF fit is higher than that obtained from the method based on the RMS of the spectrum; hence, we consider this a marginal detection.
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