Table 1.
Physical properties of the clusters analyzed in this work.
| Cluster name | RAJ2000 | DecJ2000 | z | M500 (†) | R500 (†) | RMH (‡) | LX, R500 |
|---|---|---|---|---|---|---|---|
| [h, m, s] | [deg, ′, ″] | [1014 M⊙] | [Mpc] | [kpc] | [1044 erg s−1] | ||
| 2A0335+096 | 03 38 44.4 | +09 56 34 | 0.035 | 2.3 |
0.92 | 70 | 4.4 ± 0.5 |
| RBS 797 | 09 47 00.2 | +76 23 44 | 0.345 | 6.3 |
1.16 | 120 | 41.9 ± 5.4 |
| Abell 3444 | 10 23 54.8 | −27 17 09 | 0.254 | 7.6 |
1.27 | 120 | 28.3 ± 4.0 |
| MS 1455.0+2232 | 14 57 15.1 | +22 20 34 | 0.258 | 3.5 |
0.98 | 120 | 21.1 ± 2.2 |
| RXC J1504.1−0248 | 15 04 05.4 | −02 47 54 | 0.215 | 7.0 |
0.98 | 140 | 68.4 ± 7.0 |
| RX J1532.9+3021 | 15 32 53.8 | +30 20 58 | 0.345 | 4.7 |
1.04 | 100 | 41.6 ± 4.5 |
| RX J1720.1+2637 | 17 20 12.6 | +26 37 23 | 0.164 | 6.3 |
1.24 | 140 | 17.2 ± 1.7 |
Notes. (†) Radius and total mass at a mean over-density of 500 with respect to the cosmological critical density at redshift z. (‡) Average radius of the diffuse emission defined as R
where Rmax and Rmin are the maximum and minimum radius as derived from the 3σ iso-contour emission. Bolometric X-ray luminosity measured within R500. The values are taken from Giacintucci et al. (2017) and references therein.
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