Table A.2.
Results of the STARLIGHT spectral fitting.
| Name | Balmer | Nebular | YSP | ISP | OSP | log(SFR) | ΔVSL | σSL | AV | YSP AV | Metallicity |
|---|---|---|---|---|---|---|---|---|---|---|---|
| Lines? | (per cent) | (per cent) | (per cent) | (per cent) | (M⊙ yr−1) | (km s−1) | (km s−1) | (mag) | (mag) | ||
| J0052-01 | N | 38 | 7 ± 7 | 48 ± 10 | 35 ± 15 | 0.48 ± 3.9 | −8 ± 21 | 181 ± 25 | 0.465 ± 0.14 | 3.312 ± 1.72 | S,L,H |
| J0232-08 | Y | 23 | 29 ± 2 | 24 ± 3 | 37 ± 5 | 1.52 ± 0.1 | 41 ± 8 | 164 ± 8 | 0.025 ± 0.00 | 4.057 ± 0.06 | S,S,S |
| J0731+39 | Y | 19 | 42 ± 4 | 11 ± 3 | 42 ± 4 | 0.68 ± 0.2 | 30 ± 10 | 142 ± 9 | 0.621 ± 0.03 | 2.299 ± 0.40 | L,S,H |
| J0759+50 | Y | 89 | 18 ± 2 | 15 ± 2 | 57 ± 3 | 0.94 ± 0.0 | −49 ± 7 | 146 ± 10 | 0.397 ± 0.03 | 3.182 ± 0.12 | L,S,S |
| J0802+25 | Y | 22 | 41 ± 1 | 16 ± 1 | 34 ± 3 | 1.65 ± 0.1 | −16 ± 11 | 198 ± 5 | 0.257 ± 0.04 | 3.148 ± 0.13 | S,L,L |
| J0802+46 | Y | 40 | 11 ± 5 | 13 ± 3 | 66 ± 5 | 0.86 ± 3.5 | −248 ± 10 | 171 ± 8 | 0.903 ± 0.02 | 2.922 ± 0.70 | L,H,H |
| J0805+28 | Y | 24 | 37 ± 3 | 28 ± 3 | 28 ± 2 | 0.68 ± 0.1 | 84 ± 9 | 158 ± 9 | 0.669 ± 0.02 | 0.00 | L,L,S |
| J0818+36 | N | 35 | 7 ± 4 | 33 ± 4 | 51 ± 3 | −0.06 ± 1.9 | −10 ± 13 | 181 ± 13 | 0.710 ± 0.03 | 1.970 ± 0.46 | L,S,S |
| J0841+01 | N | 30 | 31 ± 3 | 20 ± 2 | 38 ± 3 | 0.25 ± 0.2 | 36 ± 28 | 202 ± 16 | 0.865 ± 0.03 | 0.227 ± 0.15 | L,S,L |
| J0858+31 | Y | 18 | 0 ± 0 | 7 ± 2 | 83 ± 3 | … | 59 ± 4 | 158 ± 4 | 0.325 ± 0.02 | … | L,S,S |
| J0915+30 | Y | 23 | 18 ± 2 | 33 ± 3 | 39 ± 6 | 1.18 ± 0.1 | −147 ± 14 | 197 ± 11 | 0.418 ± 0.08 | 3.302 ± 0.29 | S,L,H |
| J0939+35 | N | 36 | 23 ± 2 | 19 ± 2 | 48 ± 5 | 1.26 ± 0.1 | 125 ± 16 | 235 ± 24 | 0.379 ± 0.11 | 3.747 ± 0.31 | S,L,S |
| J0945+17 | N | 57 | 76 ± 2 | 4 ± 3 | 14 ± 4 | 1.15 ± 0.1 | 133 ± 25 | 172 ± 20 | 0.003 ± 0.00 | 2.204 ± 0.18 | S,S,L |
| J1010+06 | N | 39 | 65 ± 4 | 13 ± 2 | 23 ± 3 | 1.53 ± 0.1 | 156 ± 27 | 218 ± 16 | 1.231 ± 0.03 | 2.395 ± 0.24 | L,S,S |
| J1015+00 | Y | 25 | 41 ± 2 | 0 ± 0 | 49 ± 3 | 1.66 ± 0.0 | −22 ± 17 | 168 ± 10 | 0.012 ± 0.00 | 3.915 ± 0.03 | S,S,S |
| J1016+00 | Y | 22 | 35 ± 2 | 15 ± 3 | 40 ± 4 | 1.42 ± 0.1 | −14 ± 12 | 192 ± 8 | 0.192 ± 0.04 | 3.760 ± 0.11 | S,L,H |
| J1034+60 | N | 43 | 36 ± 1 | 9 ± 2 | 45 ± 3 | 1.11 ± 0.1 | −17 ± 9 | 192 ± 6 | 0.179 ± 0.04 | 3.146 ± 0.21 | S,L,L |
| J1036+01 | Y | 13 | 31 ± 1 | 24 ± 2 | 34 ± 4 | 1.55 ± 0.1 | 24 ± 13 | 188 ± 8 | 0.443 ± 0.06 | 3.438 ± 0.16 | S,L,H |
| J1100+08 | Y | 30 | 44 ± 2 | 0 ± 0 | 54 ± 2 | 1.13 ± 0.1 | −59 ± 17 | 165 ± 9 | 0.386 ± 0.03 | 2.087 ± 0.16 | L,L,S |
| J1137+61 | N | 33 | 45 ± 2 | 0 ± 0 | 45 ± 3 | 1.35 ± 0.0 | 23 ± 13 | 237 ± 10 | 0.141 ± 0.06 | 3.858 ± 0.11 | H,L,S |
| J1152+10 | N | 43 | 25 ± 2 | 14 ± 1 | 51 ± 4 | 0.89 ± 0.1 | −57 ± 9 | 184 ± 7 | 0.373 ± 0.08 | 3.536 ± 0.24 | S,L,H |
| J1157+37 | Y | 16 | 29 ± 1 | 34 ± 3 | 27 ± 4 | 1.46 ± 0.1 | −59 ± 14 | 188 ± 9 | 0.309 ± 0.04 | 3.299 ± 0.10 | S,L,S |
| J1200+31 | N | 60 | 73 ± 2 | 0 ± 0 | 18 ± 4 | 1.61 ± 0.1 | −104 ± 21 | 157 ± 11 | 0.386 ± 0.08 | 3.465 ± 0.21 | H,H,S |
| J1218+47 | Y | 26 | 55 ± 3 | 0 ± 1 | 36 ± 5 | 1.38 ± 0.1 | 46 ± 10 | 141 ± 15 | 0.150 ± 0.05 | 3.611 ± 0.23 | S,L,S |
| J1223+08 | Y | 23 | 41 ± 2 | 28 ± 3 | 21 ± 4 | 1.22 ± 0.0 | −70 ± 16 | 162 ± 12 | 0.000 ± 0.00 | 3.411 ± 0.05 | S,S,H |
| J1238+09 | Y | 18 | 37 ± 2 | 11 ± 1 | 42 ± 4 | 1.34 ± 0.1 | 23 ± 17 | 226 ± 15 | 0.582 ± 0.08 | 3.185 ± 0.33 | S,L,S |
| J1241+61 | Y | 14 | 100 ± 3 | 0 ± 2 | 0 ± 1 | 1.96 ± 0.0 | −3 ± 11 | 140 ± 13 | 0.491 ± 0.07 | 3.626 ± 0.06 | S,S,S |
| J1244+65 | Y | 86 | 48 ± 4 | 26 ± 6 | 19 ± 4 | 1.78 ± 0.4 | 142 ± 23 | 143 ± 16 | 1.004 ± 0.31 | 3.511 ± 1.13 | S,L,S |
| J1300+54 | N | 37 | 56 ± 2 | 11 ± 3 | 26 ± 3 | 1.06 ± 0.1 | −15 ± 8 | 147 ± 6 | 0.020 ± 0.00 | 2.725 ± 0.11 | H,S,L |
| J1316+44 | N | 18 | 72 ± 2 | 1 ± 2 | 24 ± 3 | 1.10 ± 0.1 | 115 ± 16 | 148 ± 12 | 0.714 ± 0.12 | 1.492 ± 0.29 | L,S,S |
| J1347+12 | Y | 40 | 58 ± 2 | 11 ± 1 | 26 ± 3 | 1.77 ± 0.0 | 322 ± 25 | 212 ± 15 | 0.666 ± 0.07 | 3.833 ± 0.13 | S,S,H |
| J1356-02 | Y | 28 | 30 ± 4 | 17 ± 4 | 48 ± 4 | 0.40 ± 0.2 | −40 ± 14 | 133 ± 11 | 1.083 ± 0.06 | 0.718 ± 0.61 | L,H,H |
| J1356+10 | N | 37 | 27 ± 1 | 24 ± 1 | 43 ± 2 | 0.13 ± 0.0 | 100 ± 21 | 208 ± 13 | 0.778 ± 0.01 | 0.00 | L,S,L |
| J1405+40 | Y | 21 | 26 ± 3 | 22 ± 3 | 44 ± 4 | 0.77 ± 0.2 | −10 ± 8 | 121 ± 7 | 0.311 ± 0.07 | 2.166 ± 0.51 | L,S,S |
| J1430+13 | Y | 27 | 31 ± 1 | 46 ± 2 | 19 ± 2 | 0.50 ± 0.0 | −16 ± 11 | 197 ± 10 | 0.328 ± 0.02 | 0.00 | L,L,S |
| J1436+13 | N | 38 | 25 ± 2 | 21 ± 3 | 43 ± 4 | 1.40 ± 0.1 | 18 ± 14 | 192 ± 5 | 0.645 ± 0.08 | 3.226 ± 0.18 | L,H,H |
| J1437+30 | N | 34 | 50 ± 2 | 0 ± 1 | 41 ± 4 | 1.37 ± 0.2 | 62 ± 12 | 199 ± 9 | 0.533 ± 0.15 | 2.919 ± 0.56 | S,S,S |
| J1440+53 | N | 8 | 92 ± 2 | 4 ± 2 | 3 ± 2 | 1.40 ± 0.1 | 101 ± 17 | 143 ± 18 | 0.462 ± 0.26 | 3.922 ± 0.56 | H,L,L |
| J1455+32 | Y | 28 | 32 ± 1 | 29 ± 3 | 29 ± 4 | 1.10 ± 0.0 | −14 ± 7 | 153 ± 7 | 0.333 ± 0.04 | 3.423 ± 0.10 | S,L,H |
| J1509+04 | Y | 29 | 33 ± 3 | 10 ± 4 | 49 ± 4 | 0.43 ± 0.2 | 134 ± 11 | 144 ± 14 | 0.890 ± 0.04 | 0.00 | L,S,S |
| J1517+33 | N | 149 | 22 ± 6 | 28 ± 6 | 41 ± 5 | 1.63 ± 1.0 | 62 ± 21 | 228 ± 15 | 1.169 ± 0.06 | 4.112 ± 0.23 | S,L,H |
| J1533+35 | N | 23 | 30 ± 5 | 30 ± 6 | 30 ± 7 | 0.72 ± 0.4 | −16 ± 17 | 149 ± 13 | 0.618 ± 0.17 | 2.343 ± 0.78 | S,L,H |
| J1548-01 | N | 24 | 88 ± 3 | 6 ± 4 | 1 ± 1 | 1.16 ± 0.0 | 39 ± 17 | 213 ± 21 | 0.265 ± 0.08 | 1.327 ± 0.47 | H,S,L |
| J1558+35 | N | 38 | 44 ± 3 | 12 ± 3 | 35 ± 4 | 1.48 ± 0.0 | −9 ± 11 | 118 ± 12 | 0.075 ± 0.02 | 3.816 ± 0.07 | H,S,S |
| J1624+33 | N | 20 | 50 ± 2 | 8 ± 4 | 32 ± 5 | 1.32 ± 0.0 | 53 ± 13 | 153 ± 10 | 0.081 ± 0.01 | 3.617 ± 0.07 | S,S,H |
| J1653+23 | N | 36 | 43 ± 1 | 15 ± 2 | 32 ± 3 | 1.48 ± 0.0 | 14 ± 12 | 198 ± 10 | 0.089 ± 0.01 | 3.503 ± 0.05 | S,H,S |
| J1713+57 | Y | 31 | 27 ± 2 | 21 ± 2 | 44 ± 2 | 1.26 ± 0.1 | 32 ± 11 | 163 ± 10 | 0.604 ± 0.05 | 3.036 ± 0.23 | L,S,H |
| J2154+11 | Y | 25 | 12 ± 6 | 19 ± 4 | 62 ± 6 | 0.71 ± 0.9 | −13 ± 14 | 194 ± 13 | 0.656 ± 0.04 | 2.591 ± 0.43 | L,S,H |
Notes. Column 1 gives the abbreviated name, column 2 denotes whether the higher order Balmer absorption lines were detected before nebular subtraction, and column 3 gives the percentage of the total flux attributed to the nebular component below 3646 Å. Where possible, the flux was measured in the wavelength bin 3540 – 3640 Å, otherwise it was measured between the shortest wavelength and 3640Å. Columns 4, 5, and 6 give the percentage of the total flux, before reddening is applied, associated with the YSP, ISP, and OSP respectively, measured in the normalising bin (4190 – 4210 Å). Columns 8 and 9 give the AV values used by STARLIGHT for the fitting and the additional reddening that was applied to templates with ages < 7 Myr (where applicable). The final column gives the metallicity allocated to the OSP, ISP, and YSP respectively: H=super-solar, S=Solar, and L=sub-solar.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.