Table 2
Properties of radio galaxies in Fig. 3 and their respective host galaxies.
| EMU ES | Our label | Host name | Redshift | Extent of radio lobes | ||
|---|---|---|---|---|---|---|
| name | (in Fig. 3) | z | LAS | LLS | Comments | |
| [arcmin] | [kpc] | |||||
| J0626–5341 | N1 | ESO 161-IG 007 NED02 | 0.0551 | 5.35 | 346 | FR I in A3391 |
| J0626–5433 | S1 | WISEA J062649.57–543234.4 | 0.0520 | 6.07 | 372 | PKS 0625–545, in A3395 |
| J0626–5432 | S2 | – ? | – | 5.52 | – | relic/remnant in A3395 |
| J0625–5427 | S3 | WISEA J062557.04–542750.4 ? | 0.0603 | 3.25 | 229 | remnant/relic in A3395 |
| J0622–5334 | F1 | WISEA J062255.56–533434.5 | 0.0567 | 5.71 | 379 | asym. FR II?, PMN 0622–5334 |
| J0621–5241 | F2 | 2MASX J06214330–5241333 | 0.0511 | 6.21 | 374 | WAT, PKS 0620–52 |
| J0632–5404 | F3 | WISEA J063201.16–540457.4 | 0.193 | 5.80 | 1117 | FR II plume |
Notes. Columns are (1) a shortened name where ‘EMU ES’ stands for Evolutionary Map or the Universe Early Science Source, (2) the source label according to Figs. 1 and 3, (3) the name of the optical host galaxy, (4) its spectroscopic redshift, (5) its largest angular size (LAS) measured in a straight line between opposite ends of the detectable radio emission, (6) its largest projected linear size (LLS) assuming the cosmological parameters listed at the end of Sect. 1.
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