Table 3.
Inferred quantities for the VACA LoCA sample clusters under the assumption of a universal pressure profile (Arnaud et al. 2010).
| Cluster ID | zphot | λ | r500 | θ500 | Ysph(< r500) | Ycyl(< r500) | M500 | σeff |
|---|---|---|---|---|---|---|---|---|
| – | – | (Mpc) | (arcmin) | 10−5 Mpc2 | 10−5 Mpc2 | (1014 M⊙) | – | |
| Significant detection | ||||||||
| MOO J0129−1640 |
 |
49 ± 7 |
 |
 |
 |
 |
 |
7.77 |
| MOO J0345−2913 |
 |
53 ± 7 |
 |
 |
 |
 |
 |
5.32 |
| MOO J0917−0700(a) |
 |
58 ± 7 |
 |
 |
 |
 |
 |
4.26 |
 |
 |
 |
 |
 |
||||
| MOO J1139−1706 |
 |
53 ± 7 |
 |
 |
 |
 |
 |
3.81 |
| MOO J1342−1913 |
 |
41 ± 6 |
 |
 |
 |
 |
 |
4.53 |
| MOO J1414+0227 |
 |
41 ± 7 |
 |
 |
 |
 |
 |
6.99 |
| MOO J2146−0320(a) |
 |
50 ± 7 |
 |
 |
 |
 |
 |
5.35 |
 |
 |
 |
 |
 |
||||
| Non-detection | ||||||||
| MOO J0903+1310 |
 |
29 ± 5 | 0.30+0.05 | 0.59+0.10 | 0.04+0.06 | 0.05+0.07 | 0.30+0.18 | – |
| MOO J1223+2420(b) |
 |
51 ± 7 |
 |
 |
 |
 |
 |
2.40 |
| MOO J2147+1314 |
 |
38 ± 6 |
 |
 |
 |
 |
 |
1.26 |
Notes. See Sect. 4 for more details about the effective significance estimate σeff. The photometric redshift zphot and infrared richness λ are taken from Gonzalez et al. (2019).
The two mass values provided for MOO J0917−0700 and MOO J2146−0320 correspond to the masses of each of the individual SZ components detected.
The SZ signal from MOO J1223+2420 has significant contamination from an FR II radio galaxy at the center of the cluster (see Sect. 4.3 for a discussion).
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