Table A.1
Candidate associations of radio AGNs and X-ray clusters from the catalogue of Finoguenov et al. 27.
RAcl | Deccl | z cl | Distance (arcsec) | Δz |
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0.7 ≤ z< 1 | ||||||
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150.41386 | 1.84759 | 0.969 | 40.176 | 0.015 | 2.9883 × 1043 | 25.68 |
150.27736 | 2.05303 | 0.908 | 41.112 | –0.0521 | 9.6268 × 1042 | 23.76 |
150.02382 | 2.20323 | 0.942 | 7.1856 | 0.0988 | 1.9325 × 1043 | 23.35 |
149.64966 | 2.20925 | 0.954 | 0.120744 | –0.0165 | 1.7111 × 1043 | 24.34 |
150.21454 | 2.28010 | 0.881 | 26.3124 | –0.0419 | 1.3734 × 1043 | 24.59 |
149.95262 | 2.34188 | 0.942 | 0.0144 | 0.0156 | 1.5213 × 1043 | 23.47 |
149.95262 | 2.34188 | 0.942 | 41.76 | –0.0002 | 1.5213 × 1043 | 24.16 |
149.92926 | 2.40902 | 0.874 | 0.0072 | –0.0044 | 8.4425 × 1042 | 23.58 |
149.63988 | 2.34912 | 0.951 | 41.112 | –0.0369 | 3.2975 × 1043 | 24.06 |
149.62355 | 2.39918 | 0.845 | 0.108072 | 0.0051 | 1.9522 × 1043 | 24.31 |
150.15298 | 2.39447 | 0.899 | 26.01 | 0.0193 | 9.4442 × 1042 | 23.64 |
149.66927 | 2.47365 | 0.957 | 11.4408 | –0.0044 | 1.8343 × 1043 | 23.92 |
149.56174 | 2.42195 | 0.846 | 0.0144 | 0.0332 | 1.7645 × 1043 | 24.20 |
150.00713 | 2.45343 | 0.731 | 0.1476 | 0.0229 | 5.2795 × 1042 | 24.15 |
149.92343 | 2.52499 | 0.729 | 30.8016 | 0.0016 | 1.1257 × 1044 | 23.74 |
150.10533 | 2.72392 | 0.727 | 2.39364 | –0.0023 | 6.9659 × 1042 | 23.89 |
149.91772 | 2.70088 | 0.889 | 3.00132 | –0.0355 | 2.1160 × 1043 | 24.28 |
150.58397 | 2.32155 | 0.720 | 46.116 | 0.0182 | 4.2323 × 1042 | 23.39 |
150.05057 | 2.13923 | 0.959 | 1.09008 | 0.1189 | 5.7184 × 1042 | 24.19 |
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1 ≤ z ≤ 2 | ||||||
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150.76245 | 1.79362 | 1.258 | 10.4004 | –0.0051 | 5.5689 × 1043 | 26.43 |
149.51855 | 2.09959 | 1.382 | 48.096 | 0.1839 | 7.8229 × 1043 | 24.00 |
150.59309 | 2.53890 | 1.045 | 7.056 | –0.1063 | 3.1937 × 1043 | 23.63 |
149.59763 | 2.44004 | 1.168 | 10.4076 | –0.023 | 2.6946 × 1043 | 26.86 |
150.57024 | 2.49864 | 1.146 | 17.586 | –0.0083 | 2.5386 × 1043 | 24.13 |
150.12646 | 1.99926 | 1.019 | 13.644 | –0.1744 | 1.2897 × 1043 | 23.65 |
Notes. RAcl, Deccl and zcl are the coordinates of the cluster centre. Column 4 is the distance between the cluster centre and the source of the AGN sample considered on the plane of the sky, while Col. 5 is the distance in redshift between the two. LX( [ 0.1−2.4 ] keV) and log (L1.4 GHz) are the X-ray and 1.4 GHz luminosities.
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