Table 1.
List of cluster properties.
| Name | Sample | NGG, GC | Nlit | NM (Nm) |
 |
σlos | r200 | M200 | Refs. |
|---|---|---|---|---|---|---|---|---|---|
| [km s−1] | [Mpc] | [1014 M⊙] | |||||||
| SpARCS0034 | GCLASS | 67 | – | 31.5 (32) | 0.8673 ± 0.0005 | 405 ± 51 | 0.58, 0.58, 0.61 | 0.6 ± 0.2 | |
| SpARCS0035 | GGGC | 129 | – | 28.0 (29) | 1.3357 ± 0.0013 | 840 ± 111 | 0.93, 0.90, 1.01 | 3.8 ± 1.5 | |
| SpARCS0036 | GCLASS | 70 | – | 43.0 (48) | 0.8697 ± 0.0008 | 799 ± 82 | 1.12, 1.06, 1.21 | 3.6 ± 1.1 | |
| SpARCS0215 | GCLASS | 61 | – | 43.0 (44) | 1.0035 ± 0.0007 | 656 ± 70 | 0.85, 0.88, 0.89 | 2.4 ± 0.8 | |
| SpARCS0335 | GOGREEN | 66 | 67 | 23.0 (27) | 1.3690 ± 0.0010 | 542 ± 75 | 0.67, 0.69, 0.76 | 1.8 ± 0.7 | a |
| SpARCS1047 | GCLASS | 68 | – | 29.0 (29) | 0.9566 ± 0.0008 | 668 ± 89 | 0.91, 0.91, 0.99 | 2.5 ± 1.0 | |
| SpARCS1051 | GGGC | 185 | – | 42.0 (42) | 1.0344 ± 0.0007 | 689 ± 75 | 0.88, 0.84, 0.95 | 2.2 ± 0.7 | |
| SpARCS1613 | GCLASS | 96 | – | 68.5 (86) | 0.8701 ± 0.0009 | 1185 ± 90 | 1.59, 1.54, 1.72 | 11.1 ± 2.5 | |
| SpARCS1616 | GGGC | 214 | – | 59.5 (60) | 1.1562 ± 0.0007 | 782 ± 71 | 0.92, 0.92, 1.00 | 3.3 ± 0.9 | |
| SpARCS1634 | GGGC | 190 | – | 63.0 (70) | 1.1780 ± 0.0007 | 715 ± 60 | 0.85, 0.85, 0.88 | 2.7 ± 0.7 | |
| SpARCS1638 | GGGC | 174 | – | 56.0 (56) | 1.1938 ± 0.0006 | 564 ± 53 | 0.71, 0.73, 0.74 | 1.7 ± 0.5 | |
| SPT0205 | GOGREEN | 65 | 5 | 28.0 (28) | 1.3227 ± 0.0010 | 678 ± 91 | 0.76, 0.85, 0.80 | 3.1 ± 1.2 | b |
| SPT0546 | GOGREEN | 63 | 40 | 62.0 (67) | 1.0669 ± 0.0009 | 977 ± 84 | 1.17, 1.15, 1.22 | 5.8 ± 1.5 | c |
| SPT2106 | GOGREEN | 67 | 14 | 43.0 (50) | 1.1307 ± 0.0012 | 1055 ± 106 | 1.23, 1.21, 1.24 | 7.3 ± 2.2 | d |
Notes. GOGREEN, GGGC, and GCLASS identify the data base: GOGREEN-only data, GOGREEN and GCLASS data, and GCLASS-only data, respectively. NGG, GC is the number of objects with good-quality redshifts from either GOGREEN or GCLASS, and Nlit the number of objects with good-quality redshifts available in the literature for galaxies that do not have redshifts from either GOGREEN or GCLASS. The total number of galaxies with redshifts Ntot is obtained by the sum NGG, GC + Nlit. The references to the literature data are given in the last column: a: Nantais et al. (2016), b: Stalder et al. (2013), c: Sifón et al. (2016), d: Foley et al. (2011). NM is the weighted number of members among the Ntot objects (see text). In parentheses we list Nm, the number of galaxies that would be considered as members by at least one of the two cluster membership algorithms used in this analysis (see text for more details). 
and σlos are the weighted estimates of the cluster mean redshift and velocity dispersion, obtained by using the galaxy membership weights (1σ errors are listed). The r200 column lists three estimates for each cluster, obtained respectively by the Clean procedure (r200, C), and by MAMPOSSt (r200, Mt and r200, Mc) using two different mass and anisotropy profiles (see text for more details). Uncertainties on r200 are not listed as they are proportional to the fractional uncertainties on σlos. The M200 column lists the values obtained from r200, Mt, with uncertainties estimated as 3 times the fractional error on σlos.
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