Table 2.
Properties and literature information of the selected sample of non-merging massive clusters.
| Name | z | Scale | M500 | K0 | X-ray | Radio | Telescope & frequency | Ref. |
|---|---|---|---|---|---|---|---|---|
| (kpc/′′) | (1014 M⊙) | (keV cm2) | ||||||
| RXCJ0142.0+2131 | 0.280 | 4.28 | 6.07 | 131 | nCC | UL | GMRT: 235/610 MHz | 1 |
| A478 | 0.088 | 1.66 | 7.06 | 8 | CC | MH | VLA: 1.4 GHz | 2 |
| PSZ1G139.61+24 | 0.270 | 4.17 | 7.09 | 10 | CC | cMH | GMRT: 610 MHz | 3 |
| A1413 | 0.143 | 2.53 | 5.98 | 64 | nCC | cMH | VLA: 1.4 GHz | 4 |
| A1423 | 0.214 | 3.50 | 6.09 | 27 | CC | UL | GMRT: 610 MHz | 5 |
| A1576 | 0.302 | 4.51 | 5.98 | 186 | nCC | UL | GMRT: 610 MHz | 1 |
| RXJ1720.1+2638 | 0.164 | 2.84 | 6.34 | 21 | CC | MH | GMRT: 317/617 MHz, 1.28 GHz | 6 |
| VLA: 1.5, 4.9, 8.4 GHz | 6 | |||||||
| A2261 | 0.224 | 3.63 | 7.39 | 61 | nCC | H | VLA: 1.4 GHz | 7 |
| A2390 | 0.234 | 3.75 | 9.48 | 15 | CC | H | VLA: 1.4 GHz | 7 |
Notes. Column 1: name of the cluster; Col. 2: redshift; Col. 3: angular to physical scale conversion at the cluster redshift; Col. 4: mass within the radius enclosing a mean density of 500 times the critical density (Planck Collaboration XXIX 2014); Col. 5: core entropy from X-ray data (Giacintucci et al. 2017); Col. 6: presence of a cool core (CC) from X-ray data (Giacintucci et al. 2017); Col. 7: presence of radio diffuse emission as present in the literature (UL = upper limit; MH = mini halo; cMH = candidate mini halo; H = halo); Col. 8: observations present in the literature; Col. 9: radio references.
References. (1) Kale et al. 2013; (2) Giacintucci et al. 2014b; (3) Giacintucci et al. 2017; (4) Govoni et al. 2009 (5) Venturi et al. 2008; (6) Giacintucci et al. 2014a; (7) Sommer et al. 2017.
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