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Caption: Fig. 2.
Chandra spectra of the sample of X‐ray–weak quasars. The shaded region represents the X‐ray spectrum expected assuming ﹩\alpha _{\mathrm{OX}\,}=1.55﹩ and ﹩\Gamma =1.8﹩. ROSAT upper limits are shown for the three sources having fluxes significantly higher than those in ROSAT observations.
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