Open Access
Table A.4.
Continued.
| Col. name | Description |
|---|---|
| MASS_ff | log M/M⊙ where M is the stellar mass derived from the ffa SED fit (Sect.6.4). |
| LERR_MASS_ff | Lower 1σ percentile of log M/M⊙ |
| HERR_MASS_ff | Upper 1σ percentile of log M/M⊙ |
| SFR_ff | log SFR/M⊙yr−1 where SFR is the star formation rate at 100 Myr lookback time as derived from the ffa SED fit (Sect.6.4). |
| LERR_SFR_ff | Lower 1σ percentile of log SFR/M⊙yr−1 |
| HERR_SFR_ff | Upper 1σ percentile of log SFR/M⊙yr−1 |
| LINE_SNR_MAX | name of emission or absorption line with max S/N b |
| SNR_MAX | max S/N |
| FLUX_MAX | flux of the line with max S/N (10−20erg s−1 cm−2) |
| lll_EMI_FLUX | flux of the lllc emission line (10−20erg s−1 cm−2) |
| lll_EMI_SNR | S/N of the lll emission line |
| lll_EMI_EQW | Rest frame equivalent width of the lll emission line (Å) |
| lll_EMI_VD | Rest frame velocity dispersiond of the lll emission line (km s−1) |
| lll_ABS_FLUX | flux of the lllb absorption line (10−20erg s−1 cm−2) |
| lll_ABS_SNR | S/N of the lll absorption line |
| lll_ABS_EQW | Rest frame equivalent width of the lll absorption line (Å) |
| lll_ABS_VD | Rest frame velocity dispersionc of the lll absorption line (km s−1) |
Notes.
b
b at the end of line name indicate a blend (e.g., OII3727b is the sum of the [O II]λλ3726,3729 doublet)
c
see table D.1 for line names
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