  We present the distance-calibrated spectral energy distribution (SED) of the
d/sdL7 SDSS J14162408+1348263A (J1416A) and an updated SED for SDSS
J14162408+1348263B (J1416B). We also present the first retrieval analysis of
J1416A using the Brewster retrieval code base and the second retrieval of
J1416B. We find that the primary is best fit by a non-grey cloud opacity with a
power-law wavelength dependence, but is indistinguishable between the type of
cloud parameterization. J1416B is best fit by a cloud-free model, consistent
with the results from Line et al. (2017). Most fundamental parameters derived
via SEDs and retrievals are consistent within 1 sigma for both J1416A and
J1416B. The exceptions include the radius of J1416A, where the retrieved radius
is smaller than the evolutionary model-based radius from the SED for the deck
cloud model, and the bolometric luminosity which is consistent within 2.5 sigma
for both cloud models. The pair's metallicity and Carbon-to-Oxygen (C/O) ratio
point towards formation and evolution as a system. By comparing the retrieved
alkali abundances while using two opacity models, we are able to evaluate how
the opacities behave for the L and T dwarf. Lastly, we find that relatively
small changes in composition can drive major observable differences for lower
temperature objects.
