  Black Hole measurements have grown significantly in the new age of
gravitation wave astronomy from LIGO observations of binary black hole mergers.
As yet unobserved massive ultralight bosonic fields represent one of the most
exciting features of Standard Model extensions, capable of providing solutions
to numerous paradigmatic issues in particle physics and cosmology. In this work
we explore bounds from spinning astrophysical black holes and their angular
momentum energy transfer to bosonic condensates which can form surrounding the
black hole via superradiant instabilities. Using recent analytical results we
perform a simplified analysis with a generous ensemble of black hole parameter
measurements where we find superradiance very generally excludes bosonic fields
in the mass ranges; spin-0: ${\scriptsize \{ 3.8\times10^{-14}\ {\rm eV} \leq
\mu_0 \leq 3.4\times10^{-11}\ {\rm eV}, 5.5\times10^{-20}\ {\rm eV} \leq \mu_0
\leq 1.3\times10^{-16}\ {\rm eV}, 2.5\times10^{-21}\ {\rm eV} \leq \mu_0 \leq
1.2\times10^{-20}\ {\rm eV}\}}$, spin-1: ${\scriptsize \{ 6.2\times10^{-15}\
{\rm eV} \leq \mu_1 \leq 3.9\times10^{-11}\ {\rm eV}, 2.8\times10^{-22}\ {\rm
eV} \leq \mu_1 \leq 1.9\times10^{-16}\ {\rm eV} \}}$ and spin-2: ${\scriptsize
\{ 2.2\times10^{-14}\ {\rm eV} \leq \mu_2 \leq 2.8\times10^{-11}\ {\rm eV},
1.8\times10^{-20}\ {\rm eV} \leq \mu_2 \leq 1.8\times10^{-16}\ {\rm eV},
6.4\times10^{-22}\ {\rm eV} \leq \mu_2 \leq 7.7\times10^{-21}\ {\rm eV} \}}$
respectively. We also explore these bounds in the context of specific
phenomenological models, specifically the QCD axion, M-theory models and fuzzy
dark matter sitting at the edges of current limits. In particular we include
recent measurements of event GW190521 and M87* used to constrain both the
masses and decay constants of axion like fields. Finally we comment a simple
example of a spectrum of fields for the spin-0 and spin-1 cases.
