  OTS44 is one of only four free-floating planets known to have a disk. We have
previously shown that it is the coolest and least massive known free-floating
planet ($\sim$12 M$_{\rm Jup}$) with a substantial disk that is actively
accreting. We have obtained Band 6 (233 GHz) ALMA continuum data of this very
young disk-bearing object. The data shows a clear unresolved detection of the
source. We obtained disk-mass estimates via empirical correlations derived for
young, higher-mass, central (substellar) objects. The range of values obtained
are between 0.07 and 0.63 M$_{\oplus}$ (dust masses). We compare the properties
of this unique disk with those recently reported around higher-mass (brown
dwarfs) young objects in order to infer constraints on its mechanism of
formation. While extreme assumptions on dust temperature yield disk-mass values
that could slightly diverge from the general trends found for more massive
brown dwarfs, a range of sensible values provide disk masses compatible with a
unique scaling relation between $M_{\rm dust}$ and $M_{*}$ through the
substellar domain down to planetary masses.
