Table E.1.
Stellar mass-metallicity relation for different SFH types.
[M/H]M | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|
All | ST-SFH | LT-SFH | ||||||||||
log10M⋆[M⊙] | n | p50 | p16 | p84 | n | p50 | p16 | p84 | n | p50 | p16 | p84 |
(a) Voids | ||||||||||||
8.25 | 4 | - | - | - | 1 | - | - | - | 3 | - | - | - |
8.75 | 56 | -0.77±0.03 | -1.12 | -0.36 | 8 | - | - | - | 48 | -0.88±0.04 | -1.18 | -0.48 |
9.25 | 159 | -0.627±0.017 | -1.01 | -0.20 | 40 | -0.25±0.04 | -0.42 | -0.07 | 119 | -0.752±0.019 | -1.06 | -0.28 |
9.75 | 363 | -0.247±0.009 | -0.70 | 0.01 | 127 | -0.076±0.016 | -0.34 | 0.08 | 236 | -0.403±0.012 | -0.77 | -0.05 |
10.25 | 309 | -0.000±0.009 | -0.29 | 0.21 | 187 | 0.038±0.011 | -0.16 | 0.24 | 122 | -0.072±0.014 | -0.49 | 0.16 |
10.75 | 91 | 0.208±0.012 | -0.07 | 0.36 | 68 | 0.279±0.013 | 0.06 | 0.37 | 23 | 0.05±0.03 | -0.20 | 0.14 |
11.25 | 4 | - | - | - | 3 | - | - | - | 1 | - | - | - |
(b) Filaments & walls | ||||||||||||
8.25 | 18 | -0.92±0.05 | -1.24 | -0.21 | 3 | - | - | - | 15 | -0.95±0.06 | -1.28 | -0.58 |
8.75 | 160 | -0.737±0.018 | -1.16 | -0.31 | 40 | -0.49±0.04 | -0.73 | -0.05 | 120 | -0.865±0.021 | -1.20 | -0.43 |
9.25 | 649 | -0.519±0.009 | -1.01 | -0.13 | 159 | -0.255±0.017 | -0.57 | 0.05 | 490 | -0.648±0.01 | -1.06 | -0.24 |
9.75 | 1600 | -0.211±0.004 | -0.66 | 0.04 | 643 | -0.080±0.006 | -0.27 | 0.11 | 957 | -0.374±0.006 | -0.81 | -0.05 |
10.25 | 2216 | 0.031±0.003 | -0.24 | 0.23 | 1273 | 0.073±0.004 | -0.12 | 0.27 | 943 | -0.056±0.005 | -0.42 | 0.15 |
10.75 | 1593 | 0.223±0.003 | 0.00 | 0.37 | 1150 | 0.277±0.003 | 0.07 | 0.38 | 443 | 0.111±0.006 | -0.13 | 0.24 |
11.25 | 213 | 0.347±0.007 | 0.22 | 0.39 | 184 | 0.370±0.007 | 0.24 | 0.39 | 29 | 0.241±0.022 | 0.10 | 0.28 |
(c) Clusters | ||||||||||||
8.25 | 2 | - | - | - | 0 | - | - | - | 2 | - | - | - |
8.75 | 41 | -0.55±0.03 | -0.96 | -0.16 | 13 | -0.18±0.06 | -0.40 | -0.05 | 28 | -0.67±0.04 | -1.06 | -0.30 |
9.25 | 265 | -0.23±0.01 | -0.60 | -0.01 | 113 | -0.146±0.014 | -0.33 | 0.05 | 152 | -0.333±0.015 | -0.85 | -0.07 |
9.75 | 972 | -0.054±0.004 | -0.27 | 0.16 | 527 | -0.012±0.005 | -0.20 | 0.19 | 445 | -0.108±0.007 | -0.42 | 0.10 |
10.25 | 1282 | 0.148±0.003 | -0.06 | 0.29 | 861 | 0.190±0.004 | -0.02 | 0.32 | 421 | 0.089±0.006 | -0.15 | 0.21 |
10.75 | 706 | 0.292±0.004 | 0.13 | 0.38 | 542 | 0.319±0.004 | 0.18 | 0.39 | 164 | 0.166±0.009 | -0.00 | 0.26 |
11.25 | 89 | 0.376±0.008 | 0.27 | 0.39 | 83 | 0.379±0.008 | 0.29 | 0.39 | 6 | - | - | - |
Notes. Stellar mass-metallicity relation for all the galaxies regardless of their SFH type (left multi-column), galaxies with ST-SFH (centre multi-column), and galaxies with LT-SFH (right multi-column) in voids (a), filaments & walls (b), and clusters (c). The stellar mas-metallicity relation is derived as the 50th percentile (p50) of the distribution, together with the error of the mean, inside each stellar mass bin. The 16th (p16) and 84th (p84) percentiles represent the dispersion of the stellar mass-metallicity relation. The number of galaxies (n) inside each stellar mas bin is also reported.
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