Table A.1.
Depletion parameters computed on mass bins for four different redshifts and radii.
Least massive subsample | Most massive subsample | ||||||||
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z | R500,c | 3R500,c | 5R500,c | 10R500,c | R500,c | 3R500,c | 5R500,c | 10R500,c | |
2.79 | 5.8 × 1012 ≤ M500,c/M⊙ ≤ 9.7 × 1012 | 2.5 × 1013 ≤ M500,c/M⊙ ≤ 5.0 × 1013 | |||||||
Ybar |
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Ygas |
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Yhot |
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Ycold |
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Ystar |
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Ztot |
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1.71 | 1.2 × 1013 ≤ M500,c/M⊙ ≤ 3.4 × 1013 | 6.0 × 1013 ≤ M500,c/M⊙ ≤ 1.5 × 1014 | |||||||
Ybar |
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Ygas |
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Yhot |
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Ycold |
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Ystar |
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Ztot |
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0.67 | 6.0 × 1013 ≤ M500,c/M⊙ ≤ 1.0 × 1014 | 2.3 × 1014 ≤ M500,c/M⊙ ≤ 4.6 × 1014 | |||||||
Ybar |
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Ygas |
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Yhot |
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Ycold |
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Ystar |
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Ztot |
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0.25 | 6.0 × 1013 ≤ M500,c/M⊙ ≤ 1.9 × 1014 | 4.6 × 1014 ≤ M500,c/M⊙ ≤ 7.5 × 1014 | |||||||
Ybar |
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Ygas |
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Yhot |
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Ycold |
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Ystar |
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Ztot |
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Notes. Baryons (Ybar), gas (Ygas), hot-gas-phase (Yhot), cold-gas-phase (Ycold), and stellar (Ystar) depletion parameters and gas metallicity (Ztot) computed at four different radii (1, 3, 5 and 10 times ) for the least massive subsample (left side) and the most massive subsample (right side) at each of the four different redshifts (2.79, 1.70, 0.67 and 0.25). Errors are given as 16th and 84th distribution percentiles. We note that the depletion parameters are computed within the given radii, differently from the metallicity values, which are given within a spherical shell (considering the same reference radii).
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