Table A.1.
List of galaxy clusters hosting a central radio galaxy classified as a GPS source and without evidence for extended radio emission.
| Object | RA | DEC | z | kpc/″ | νp | LLS | tkin |
|---|---|---|---|---|---|---|---|
| [GHz] | [pc] | [yr] | |||||
| RX J1350+0940 | 13:50:22.1 | +09:40:10.6 | 0.133 | 2.4 | 3.9 | 90 | 7 × 102 |
| Abell 1885 | 14:13:43.73 | +43:39:45.0 | 0.088 | 1.6 | 2.5 | - | - |
| ClG J0242-2132 | 02:42:35.9 | -21:32:26 | 0.314 | 4.6 | 0.8 | 200 | 1.6 × 103 |
| RX J2341+0018 | 23:41:6.8 | +00:18:34.1 | 0.277 | 4.2 | 0.4 | - | - |
| RX J0132-0804 | 01:32:41.1 | -08:04:06 | 0.148 | 2.6 | 0.1 | - | - |
Notes. The two objects in bold are the focus of this article. (1) Object name; (2) right ascension; (3) declination; (4) redshift; (5) conversion between physical and angular scales at the object’s redshift; (6) rest-frame peak frequency (from Hogan et al. 2015b); (7) largest linear size from VLBA data (see Charlot et al. 2020); and (8) kinematic age of the source (LLS/2v) assuming an expansion speed of v = 0.2c.
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