Table 1.
Sample of galaxy clusters with radio relics and detected underlying shocks.
| Cluster name | RAJ2000 | DecJ2000 | M500 | z | NH | Instrument | Ref. |
|
|---|---|---|---|---|---|---|---|---|
| (h,m,s) | (°,′,″) | (1014 M⊙) | (1020 cm−2) | R | X | |||
| A2744 | 00 14 19 | −30 23 22 | 9.56 | 0.308 | 1.46 | XMM-Newton | (1) | (2) |
| A115 | 00 55 60 | +26 22 41 | 7.20 | 0.197 | 6.38 | Chandra | (3) | (3) |
| El Gordo | 01 02 53 | −49 15 19 | 8.80 | 0.870 | 1.78 | Chandra | (4) | (4) |
| A521 | 04 54 09 | −10 14 19 | 6.90 | 0.253 | 6.06 | Chandra | (5) | (6) |
| A3376 | 06 01 45 | −39 59 34 | 2.27 | 0.046 | 5.81 | XMM-Newton | (7) | (8) |
| Toothbrush cluster | 06 03 13 | +42 12 31 | 11.1 | 0.225 | 33.4 | Chandra | (9) | (10) |
| Bullet cluster | 06 58 31 | −55 56 49 | 12.4 | 0.296 | 6.43 | Chandra | (11) | (12) |
| RXC J1314.4-2515 | 13 14 28 | −25 15 41 | 6.15 | 0.247 | 8.91 | XMM-Newton | (13) | (14) |
| A2146 | 15 56 09 | +66 21 21 | 3.85 | 0.234 | 3.35 | Chandra | (15) | (16) |
| Sausage cluster | 22 42 53 | +53 01 05 | 7.97 | 0.192 | 46.4 | Chandra | (17) | (18) |
Notes. Reported values of M500 (mass within a radius that encloses a mean overdensity of 500 with respect to the critical density at the cluster redshift) and NH (hydrogen column density) are taken from Planck Collaboration XXIX (2014) and Willingale et al. (2013), respectively. For the Sausage Cluster, M500 is from de Gasperin et al. (2014). Redshifts are taken from the NASA/IPAC Extragalactic Database (NED).
References. (R = radio, X = X-ray): (1) Giacintucci et al. (in prep.); (2) Eckert et al. (2016); (3) Botteon et al. (2016a); (4) Botteon et al. (2016b); (5) Giacintucci et al. (2008); (6) Bourdin et al. (2013); (7) Kale et al. (2012); (8) Urdampilleta et al. (2018); (9) van Weeren et al. (2012); (10) van Weeren et al. (2016); (11) Shimwell et al. (2014); (12) Shimwell et al. (2015); (13) Venturi et al. (2013); (14) Mazzotta et al. (2011); (15) Russell et al. (2012); (16) Hoang et al. (2019); (17) van Weeren et al. (2010); (18) Akamatsu et al. (2015).
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