Table 1.
Cluster sample.
Cluster | Coordinates | Redshift | M500, c | r500 | m140lim | log(M*, compl/M⊙) | fq vs. fq, field |
---|---|---|---|---|---|---|---|
[1014 M⊙] | [Mpc] | [mag] | [%] | ||||
SPT-CLJ0421-4845 | 04h21m16.9s, − 48° 45′40″ |
![]() |
![]() |
0.60 ± 0.04 | 23.5 | 10.54 |
![]() ![]() |
SPT-CLJ0607-4448 | 06h07m35.6s, − 44° 48′12″ | 1.401† |
![]() |
0.62 ± 0.04 | 23.5 | 10.56 |
![]() ![]() |
SPT-CLJ2040-4451 | 20h40m59.6s, − 44° 51′37″ | 1.478† |
![]() |
0.61 ± 0.04 | 23.5 | 10.60 |
![]() ![]() |
SPT-CLJ0446-4606 | 04h46m55.8s, − 46° 06′04″ |
![]() |
![]() |
0.56 ± 0.04 | 23.4 | 10.65 |
![]() ![]() |
SPT-CLJ0459-4947 | 04h59m42.5s, − 49° 47′14″ | 1.71† |
![]() |
0.53 ± 0.04 | 23.2 | 10.85 |
![]() ![]() |
Notes. Columns 1 to 5 list main cluster properties: name, coordinates, redshift, mass M500, c and scale radius r500, as indicated. Redshifts marked with a † are spectroscopic determinations from Bayliss et al. (2014), Khullar et al. (2019), Mantz et al. (2020); the remaining photometric redshifts are from S19. Columns 6 and 7 list, for each cluster, the limiting m140 magnitude and stellar mass completeness limit adopted in this work (from S19). Column 8 lists the quiescent galaxy fraction as estimated in S19 in the r < 0.7 r500 region and for stellar masses above log(M/M⊙) > 10.85 (left), and the quiescent fraction for the corresponding reference field sample (right).
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