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Table E.2.

Differences of the stellar mass-metallicity relation between galaxies in voids, filaments & walls, and clusters for different SFH types.

Δ[M/H]M

All ST-SFH LT-SFH
log10M[M] Δp50 σ Δp50 σ Δp50 σ
(a) Filaments & walls - Voids

8.25 - - - - - -
8.75 0.04±0.04 1.0 - - 0.01±0.04 0.2
9.25 0.108±0.019 5.7 -0.00±0.04 -0.0 0.104±0.021 5.0
9.75 0.04±0.01 4.0 -0.004±0.017 -0.2 0.029±0.013 2.2
10.25 0.031±0.009 3.4 0.035±0.011 3.2 0.016±0.015 1.1
10.75 0.015±0.013 1.2 -0.003±0.014 -0.2 0.06±0.03 2.0
11.25 - - - - - -
(b) Clusters - Voids

8.25 - - - - - -
8.75 0.23±0.05 4.6 - - 0.20±0.05 4.0
9.25 0.40±0.02 20.0 0.11±0.04 2.8 0.419±0.024 17.5
9.75 0.19±0.01 19.0 0.063±0.017 3.7 0.295±0.014 21.1
10.25 0.148±0.009 16.4 0.152±0.011 13.8 0.161±0.015 10.7
10.75 0.084±0.013 6.5 0.040±0.014 2.9 0.11±0.03 3.7
11.25 - - - - - -

Notes. Differences of stellar mass-metallicity relation between galaxies in filaments & walls and voids (a), and between galaxies in clusters and voids (b) 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). Δp50 represents the difference (together with its error) of the 50th percentile of the stellar mass-metallicity distribution between different large-scale environments, and σ is the ratio of the nominal value and the error or the difference.

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