Just add parameters:
Exponential Disk surface brightness: $x$, $y$, $R_{\rm d}$, $I_{\rm d}$
Sersic Bulge surface brightness: $R_{\rm b}$, $I_{\rm b}$, $n_{\rm b}$
NFW dark matter halo: $x_{\rm h}$, $y_{\rm h}$, $M_{200}$, $c_{200}$
Mass-to-light ratios: $\mu_{\rm d}$, $\mu_{\rm b}$
and so on.
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