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Table 4.

Parameters for the models shown in Figs. 1, 2, 3, 4, and 6.

Source z Ld LT/Ld Rdiss RBLR RT Pinj
M 1045 erg s−1 1015 cm 1015 cm 1015 cm 1045 erg s−1
PKS 0123+25 2.358 1.5e9 58.5 0.3 270 764 3.1e4 0.017
PKS 0123+25 no torus 2.358 1.5e9 58.5 0 225 764 0.012
PKS 0123+25 no torus 2.358 1.5e9 58.5 0 3.6e3 764 0.3
PKS 0123+25 (ψ = 1.3 ° ) 2.358 1.5e9 58.5 0.3 540 764 3.1e4 0.025
PKS 0227 − 369 new 2.115 2e9 18.2 0.5 660 427 5.6e3 0.011
PKS 0227 − 369 old 2.115 2e9 18.2 0.5 480 427 5.6e3 0.045
TXS 0458 − 020 new 2.291 8e8 10.4 0.5 144 322 2.7e3 0.11
TXS 0458 − 020 quiesc. 2.291 8e8 10.4 0.5 132 322 2.7e3 0.025
TXS 0458 − 020 “flare” 2.291 8e8 10.4 0.5 192 322 2.7e3 0.35
TXS 0458 − 020 (Γ = 7) 2.291 8e8 10.4 0.5 192 322 2.7e3 0.25

Notes. For the BLR we always assumed LBLR = 0.1Ld. For all models we assumed ψ = 0.1 = 5.7°, unless otherwise noted. For a simple geometry (a spherical torus surrounding the disk), the ratio LT/Ld corresponds to the aperture angle θT of the torus (the angle between the normal to the disk and the border of the torus): LT/Ld = cos2θT. A ratio LT/Ld = 0.3 gives θT = 57°, while LT/Ld = 0.5 gives θT = 45°.

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