Table 1
Measured properties of the 400d MMT cluster sample.
| CL 0030 | CL 0159 | CL 0230 | CL 0809 | CL 1357 | CL 1416 | CL 1641 | CL 1701 | |
| +2618 | +0030 | +1836 | +2811 | +6232 | +4446 | +4001 | +6414 | |
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| Redshift z | 0.50 | 0.39 | 0.80 | 0.40 | 0.53 | 0.40 | 0.46 | 0.45 |
| kBTX from V09a [keV] | 5.63 ± 1.13 | 4.25 ± 0.96 | 5.50 ± 1.02 | 4.17 ± 0.73 | 4.60 ± 0.69 | 3.26 ± 0.46 | 3.31 ± 0.62 | 4.36 ± 0.46 |
 from
V09a |
3.43 ± 0.41 | 2.51 ± 0.37 | 3.46 ± 0.46 | 3.69 ± 0.42 | 2.96 ± 0.29 | 2.52 ± 0.24 | 1.70 ± 0.20 | 3.28 ± 0.24 |
 from
V09a |
4.41 ± 1.33 | 2.67 ± 0.90 | 3.57 ± 0.99 | 2.96 ± 0.78 | 2.78 ± 0.62 | 1.76 ± 0.37 | 1.73 ± 0.49 | 2.66 ± 0.42 |
 from
V09a |
2.04 ± 0.19 | 1.92 ± 0.22 | 2.70 ± 0.27 | 3.98 ± 0.35 | 2.40 ± 0.18 | 3.10 ± 0.24 | 1.34 ± 0.13 | 3.20 ± 0.20 |
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 [kpc] from Paper
II |
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[kpc] from Paper II |
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| , no dilu. corr.
[kpc] |
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– | – | – | – |
| , no dilu. corr. [kpc] |
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– | – | – | – |
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 [kpc] |
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[kpc] |
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| , no dilu. corr.
[kpc] |
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– | – | – | – |
| , no dilu. corr. [kpc] |
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– | – | – | – |
[kpc] |
873 ± 85 | 821 ± 109 | 777 ± 75 | 930 ± 84 | 821 ± 92 | 819 ± 108 | 702 ± 138 | 877 ± 89 |
[kpc] |
949 ± 72 | 838 ± 105 | 785 ± 73 | 864 ± 97 | 804 ± 96 | 727 ± 138 | 706 ± 136 | 818 ± 102 |
[kpc] |
734 ± 120 | 751 ± 130 | 715 ± 88 | 954 ± 80 | 766 ± 106 | 877 ± 94 | 648 ± 161 | 870 ± 91 |
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 , using
cfit |
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| , using
cB13 |
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| , using
cfit, no dilu. corr. |
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– | – | – | – |
| , using
cB13, no dilu. corr. |
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– | – | – | – |
 , using
cB13 |
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 , using
cB13 |
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 , using
cB13 |
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 , using
cfit |
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| , using
cB13 |
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| , using
cfit, no dilu. corr. |
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– | – | – | – |
| , using
cB13, no dilu. corr. |
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– | – | – | – |
Notes.We quote the properties adopted from V09a and state the
overdensity radii and corresponding cluster masses used for Figs. 1 and 2. All
masses are in units of 1014M⊙, without
applying the E(z) factor. We state only
stochastic uncertainties, i.e. do not include systematics. The proxy-based masses
from V09a in the first part of this table are defined in Sect. 2.5, as well as the 
quoted in the second part. The third and fourth part of the table show the weak
lensing (Mwl) and hydrostatic
(Mhyd) for different cases,
respectively. By cfit and cB13 we
denote the choices for the NFW concentration parameter explained in Sect. 2.2. We refer to Sect. 4.3 for the introduction of the “no dilu. corr.” case (only
differing from the default for the first four clusters). See Table A.1 for further properties.
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