Open Access

Table B.1.

Redshifts, total sizes of radio sources, and sizes of the central detection(s).

Source name redshift angular size projected linear size angular size projected linear size
total [″] total [kpc] central region [″] central region [kpc]
Remnant

J104622+581427 - 108 864.86 - -

Six restarted candidates

J104113+580755 0.30894 ± 0.00006s 225 1022.85 3.18 14.45
J104204+573449 0.4807 ± 0.0001s 86 514.11 1.8 10.76
J104809+573010 0.31742 ± 0.00007s 179 827.88 0.9 4.17
J104842+585326 2.1685* 70 590.52* - -
J104912+575014 0.07256 ± 0.00002s 106 146.39 1 1.38
J105436+590901 0.8862 ± 0.0003s 135 1047.06 1 7.76

Twenty-eight active comparison sources

J103753+571812 - 97 776.78 - -
J103803+581833 0.6467* 80 640.64 4.4 30.42
J103840+573649 1.0657* 72 576.58 1 8.24
J103856+575247 0.10078 ± 0.00003s 144 267.98 0.9 1.68
J103913+581445 - 85 690.37 6.1 49.54
J103953+583213 1.9328 ± 0.0005s 75 629.85 0.8 6.84
J104130+575942 0.31643 ± 0.00005s 215 992.44 8 37.29
J104208+592018 0.5099 ± 0.0001s 192 1184.26 0.8 4.99
J104223+575026 0.66 ± 0.07p 67 466.66 2.04 14.40
J104320+585621 0.35294 ± 0.00005s 145 720.22 1.8 9.02
J104352+581327 0.3898 ± 0.0002s 249 1317.21 1.7 9.08
J104630+582745 0.11736 ± 0.00002s 134 283.54 6.5 13.89
J104655+572302 - 60 480.48 0.55 4.47
J104819+573515 - 75 609.15 1.4 11.37
J104843+572047 0.72 ± 0.04p 81 586.52 1.4 10.24
J104917+583627 - 85 680.68 - -
J104918+574530 0.71 ± 0.05p 120 861.84 1.8 13.09
J105117+583832 0.719* 95 760.76 - -
J105132+571115 0.31773 ± 0.00009s 155 718.43 2.2 10.28
J105137+592005 - 117 936.94 - -
J105160+570009 0.69 ± 0.04p 96 679.97 - -
J105237+573103 0.7090 ± 0.0002s 78 560.20 - -
J105326+570310 0.52 ± 0.05p 73 454.86 - -
J105342+565408 0.24 ± 0.02p 60 226.92 - -
J105426+573649 0.23 ± 0.06p 110 402.82 8.5 31.48
J105435+565500 0.72 ± 0.06p 106 764.58 - -
J105456+565220 - 118 944.94 - -
J105622+575334 1.2657* 60 480.48 - -

Notes. In Col. 1 are the source names in J2000 coordinates; Col. 2 lists redshifts of these sources determined in Jurlin et al. (2020) and Morganti et al. (2021a). Those redshifts marked with s were obtained from the optical SDSS spectrum, and the ones with p are for redshifts derived from photometry. Redshifts marked with an ‘*’ come from the LOFAR deep fields catalogue of the LH (Kondapally et al. 2021; Duncan et al. 2021). Cols. 3 – 6 list angular and projected linear sizes of the total radio emission measured inside 3σLOFAR18 contours, and the detections in the central region measured inside LOFAR-IB contours in case of one detection, while for multiple detections we measure their overall extent. Mark ‘-’ in Cols. 5 and 6 indicates non-detection of the central region. For sources with no reported redshift, we use z = 1 to estimate linear sizes.

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