Sample derived properties

Object name Log L(5400A)Log L(1 keV)Log LBol Abs Mv RL Browne RAlpha Alpha-OX
Q0003+158 45.94 45.38 46.14 -26.44 1.83 2.2 1.37
Q0003+199 44.29 43.39 45.48 -22.45 -0.55 2.0 1.47
Q0007+106 44.84 44.39 45.91 -23.89 1.79 0.89 0.4 1.33
Q0026+129 45.14 44.53 46.12 -24.50 -1.06 0.04 0.9 1.35
Q0049+171 43.99 44.00 45.20 -21.79 -0.11 > 3.25 0.6 1.20
Q0050+124 44.90 43.91 46.10 -23.94 -0.50 1.7 1.44
Q0052+251 45.04 44.59 46.34 -24.46 -0.75 1.31 1.1 1.39
Q0054+144 45.16 44.37 46.21 -24.61 -0.23 0.4 1.34
Q0121-590 44.66 44.23 45.85 -23.60 < 0.04 0.9 1.37
Q0134+329 45.55 44.96 46.92 -25.94 2.33 0.04 0.7 1.28
Q0205+024 45.03 44.14 46.17 -24.33 -0.39 > 2.67 1.2 1.53
Q0312-770 45.31 44.64 46.24 -24.97 2.64 10.98 0.1 1.16
Q0414-060 46.22 45.45 46.26 -27.12 2.71 0.5 1.42
Q0637-752 46.48 45.78 46.55 -27.78 3.56 >10.00 0.5 1.33
Q0804+761 45.01 44.33 46.16 -24.31 -0.72 1.0 1.44
Q0837-120 44.93 44.97 46.21 -24.21 2.42 0.27 0.7 1.15
Q0844+349 44.63 43.46 45.48 -23.54 <-1.22 0.6 1.60
Q0915+165 43.65 43.24 45.04 -22.56 0.02 0.3 1.23
Q0923+129 43.61 43.19 45.26 -21.81 < 0.48 0.7 1.31
Q1028+313 44.84 44.51 46.04 -23.96 2.03 1.69 0.8 1.30
Q1100+772 45.56 44.90 46.63 -25.52 1.59 0.13 1.0 1.40
Q1116+215 45.48 44.38 46.58 -25.38 -0.47 2.21 1.0 1.62
Q1137+660 46.14 45.60 46.11 -26.93 2.05 0.20 0.7 1.31
Q1146-037 44.77 45.01 45.95 -23.92 2.63 0.3 1.22
Q1202+281 44.64 44.54 46.11 -23.72 -0.19 3.61 1.1 1.26
Q1211+143 45.14 44.37 46.26 -24.42 -0.74 0.01 2.0 1.39
Q1219+755 44.51 44.13 45.45 -23.34 -0.30 0.8 1.21
Q1226+023 46.18 45.56 46.27 -27.03 3.00 2.49 0.5 1.37
Q1244+026 43.42 43.17 44.86 -21.57 -0.45 1.4 1.33
Q1307+085 45.14 44.36 46.16 -24.58 <-0.92 0.9 1.42
Q1351+695 43.20 43.54 45.18 -22.07 0.22 1.1 1.37
Q1352+183 44.95 44.07 45.93 -24.06 <-0.88 1.5 1.46
Q1407+265 46.45 45.74 46.58 -27.68 0.28 0.58 1.2 1.40
Q1416-129 44.59 44.62 45.81 -23.54 -0.18 0.29 0.9 1.26
Q1426+015 44.82 44.34 46.09 -23.88 -0.59 3.32 1.1 1.41
Q1501+106 43.95 43.75 45.34 -21.95 -0.87 0.50 0.9 1.28
Q1545+210 45.43 45.00 46.50 -25.31 1.28 0.05 0.8 1.37
Q1613+658 44.89 44.36 46.17 -24.21 -0.47 0.35 1.1 1.36
Q1635+119 44.66 43.99 45.56 -23.31 2.02 0.30 0.7 1.31
Q1704+608 45.82 44.50 46.82 -26.14 0.70 0.01 0.1 1.61
Q1721+343 45.30 45.08 46.51 -24.96 2.19 0.86 0.5 1.28
Q1803+676 44.89 44.12 45.73 -23.84 <-0.58 -0.2 1.45
Q2128-123 45.97 45.25 46.00 -26.51 3.38 >20.00 0.5 1.38
Q2130+099 44.50 43.61 45.72 -23.26 -0.47 1.73 0.8 1.52
Q2135-147 45.26 44.76 46.31 -24.96 1.76 0.12 0.7 1.25
Q2209+184 44.14 43.89 45.30 -22.99 2.21 0.8 1.32
Q2251-178 44.82 44.38 45.75 -23.85 -1.02 0.4 1.28

The values in this table are derived from this work.

L(5400A) is the 5400A monochromatic (nu Lnu) luminosity in erg/s (not erg/cm2/s as stated in the paper).

L(1 keV) is the 1 keV monochromatic (nu Lnu) luminosity in erg/s (not erg/cm2/s as stated in the paper), based on X-ray spectral fits.

LBol is the estimated bolometric luminosity in erg/s

Abs Mv is absolute visual magnitude

RL is the radio-loudness,

Browne R is the radio core-dominance pararameter (core to extended luminosity, see Orr and Browne 1982).

Alpha is the fitted X-ray spectral energy index (F prop to E**(-alpha)).

Alpha-OX is the X-ray loudness parameter: a two point spectral slope from rest frame 2500 A to 2 keV.

Fig. 2. Histograms of sample properties. Shaded bins correspond to radio-loud objects, $R_L>1.$ The absolute magnitude is calculated using the corrections of Veron and Veron (1987), but with our value of $\Omega_0$. The bolometric luminosity is derived from the observed energy distributions as described in the text. The monochromatic X-ray luminosity is $\nu L(\nu)$ at 2 keV in the rest frame, estimated from the IPC spectral fits. $R_{CD}$, the ratio of radio core to extended luminosity (Orr and Browne 1982), is an indicator of the source orientation; it was only possible to estimate this for a subset of the sources.