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Table B.1.

Main physical properties for the QSOs studied in Sect. 5.3, and for their pc-scale and galaxy-scale winds.

AGN properties
X-ray wind
Galaxy-scale wind
Parameter log(LBOL/L) log(MBH/M) vUFO NH, UFO UFO Ekin out Tracer
Units c (1024 cm−2) (LBOL/c) (1056 erg) (LBOL/c)
IRAS 05189+2524 12.22 0.11 ± 0.01 6.35 ± 1.03 OH+Na
I Zw 1 12.01 0.26 ± 0.01 0.60 ± 0.15 Na
PDS 456 13.61 ± 0.10 9.24 ± 0.17 0.25 ± 0.01 0.69 ± 0.09 CO
Mrk 231 12.60 ± 0.10 8.38 ± 0.09 0.067 ± 0.008 12.8 CO,OH
IRAS F11119+3257 12.67 ± 0.10 8.29 ± 0.15 0.25 ± 0.01 CO,OH
IRAS 17020+4544 [11.13, 11.79] 7.59 ± 0.08 0.09 (a) 51.0 CO
MCG-03-58-007 [11.62, 11.95] 8.34 ± 0.05 0.075 ± 0.01 0.78 ± 0.32 0.57 ± 0.03 CO
(b)APM 08279+5255 14.24 10.1 ± 0.4 0.18 ± 0.04 179 2.82 CO

Notes. The UFO mass rates are computed using Eq. (8) with (Ω/4π) in the range [0.1, 0.2], with the exceptions of I Zw 1 and PDS 456, for which covering fractions of 0.5 are directly measured.

(a)

The original entry from Longinotti et al. (2015) is , which we interpret as a truncated Gaussian distribution.

(b)

A magnification of μ = 4 is assumed.

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