From top to bottom: (i) Best-fit results for the simultaneous fitting of spectrum and the time delay as a function of the luminosity distance, marginalized over other model parameters; (ii) the same plot but as a function of the resulting Hubble constant; (iii) best-fit results for the spectrum alone as a function of the luminosity distance, marginalized over other parameters; and (iv) the corresponding plot for the time-delay fit alone.