Table 6: CLOUDY models for the three quasars: (1) $U=\frac{Q(H)}{4\pi r^{2} n c}$ where Q(H) is the number of hydrogen ionizing photons, r is the distance of the gas to the continuum source, n is the gas number density and c the speed of light.
Para PG PG PG

meter 1001+054 2112+059 1535+547

$N_{\rm H}$ [ ${\rm cm}^{-2}$ ] 10^23.3 10^22.8 10^22.5

$\rm U^{(1)}$ 10^2.7 10^1.7 10^1.8

$\alpha_{\rm OX}$ -1.72 -1.63 -1.72

$\alpha_{{\rm UV}}$ -0.5 -0.5 -0.5

$\alpha_{{\rm X}}$ -0.95 -0.95 -0.95

**Table 6:** CLOUDY models for the three quasars: (1) $U=\frac{Q(H)}{4\pi r^{2} n c}$ where Q(H) is the number of hydrogen ionizing photons, r is the distance of the gas to the continuum source, n is the gas number density and c the speed of light.
Para	PG	PG	PG
meter	1001+054	2112+059	1535+547
$N_{\rm H}$ [ ${\rm cm}^{-2}$ ]	10^23.3	10^22.8	10^22.5
$\rm U^{(1)}$	10^2.7	10^1.7	10^1.8
$\alpha_{\rm OX}$	-1.72	-1.63	-1.72
$\alpha_{{\rm UV}}$	-0.5	-0.5	-0.5
$\alpha_{{\rm X}}$	-0.95	-0.95	-0.95

Source LaTeX | All tables | In the text

	1 Introduction
	2 Optical and previous X-ray studies
	3 Observations and data reduction
	4 X-ray spectral analysis
	5 Spectral energy distribution
	6 Discussion
	7 Conclusions
	References