Table 1.

The RLQ sample used in this paper. The quasar properties are taken from Zhu et al. (2020).

Namezmilog L2500Ålog L5GHzlog L2keVlog Rαr|$\log (L_\mathrm{x}/L_\mathrm{x,rqq})\, ^a$|
000442.18 + 000023.31.00818.9130.2232.0826.911.74-0.56
000622.60 − 000424.41.03819.5130.0434.9427.314.76−0.541.08
001646.54 − 005151.72.24320.9430.2032.6626.352.330.030.02
001910.95 + 034844.62.02220.2630.3532.9126.532.43−0.750.10
003054.63 + 045908.42.20120.9230.1833.8126.593.49−0.570.26
Namezmilog L2500Ålog L5GHzlog L2keVlog Rαr|$\log (L_\mathrm{x}/L_\mathrm{x,rqq})\, ^a$|
000442.18 + 000023.31.00818.9130.2232.0826.911.74-0.56
000622.60 − 000424.41.03819.5130.0434.9427.314.76−0.541.08
001646.54 − 005151.72.24320.9430.2032.6626.352.330.030.02
001910.95 + 034844.62.02220.2630.3532.9126.532.43−0.750.10
003054.63 + 045908.42.20120.9230.1833.8126.593.49−0.570.26

The X-ray luminosity divided by that predicted by the LxLuv relation for RQQs (Zhu et al. 2020).

Table 1.

The RLQ sample used in this paper. The quasar properties are taken from Zhu et al. (2020).

Namezmilog L2500Ålog L5GHzlog L2keVlog Rαr|$\log (L_\mathrm{x}/L_\mathrm{x,rqq})\, ^a$|
000442.18 + 000023.31.00818.9130.2232.0826.911.74-0.56
000622.60 − 000424.41.03819.5130.0434.9427.314.76−0.541.08
001646.54 − 005151.72.24320.9430.2032.6626.352.330.030.02
001910.95 + 034844.62.02220.2630.3532.9126.532.43−0.750.10
003054.63 + 045908.42.20120.9230.1833.8126.593.49−0.570.26
Namezmilog L2500Ålog L5GHzlog L2keVlog Rαr|$\log (L_\mathrm{x}/L_\mathrm{x,rqq})\, ^a$|
000442.18 + 000023.31.00818.9130.2232.0826.911.74-0.56
000622.60 − 000424.41.03819.5130.0434.9427.314.76−0.541.08
001646.54 − 005151.72.24320.9430.2032.6626.352.330.030.02
001910.95 + 034844.62.02220.2630.3532.9126.532.43−0.750.10
003054.63 + 045908.42.20120.9230.1833.8126.593.49−0.570.26

The X-ray luminosity divided by that predicted by the LxLuv relation for RQQs (Zhu et al. 2020).

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