  We present a microlensing analysis of updated light curves in three filters,
$g$--band, $r$--band, and $H$--band, for the gravitationally lensed quasars
Q0957+561 and SBS0909+532. Both systems display prominent microlensing features
which we analyze using our Bayesian Monte Carlo technique to constrain the
quasar continuum emission region sizes in each band. We report sizes as
half-light radii scaled to a 60 degree inclination angle. For Q0957+561 we
measure $\log{(r_{1/2}/\text{cm})} = 16.54^{+0.33}_{-0.33}$,
$16.66^{+0.37}_{-0.62}$, and $17.37^{+0.49}_{-0.40}$ in $g$--, $r$--, and
$H$--band respectively. For SBS0909+532 we measure $\log{(r_{1/2}/\text{cm})} =
15.83^{+0.33}_{-0.33}$, $16.21^{+0.37}_{-0.62}$, and $17.90^{+0.61}_{-0.63}$ in
$g$--, $r$--, and $H$--band respectively. With size measurements in three bands
spanning the quasar rest frame ultraviolet to optical, we can place constraints
on the scaling of accretion disk size with wavelength,
$r\propto\lambda^{1/\beta}$. In a joint analysis of both systems we find a
slope shallower than that predicted by thin disk theory, $\beta =
0.35^{+0.16}_{-0.08}$, consistent with other constraints from multi-epoch
microlensing studies.
