  In this work, we discuss how the use of the symmetries well motivated in
physics beyond the Standard model (BSM) can guarantee the high quality axions.
We avoid to introduce symmetries only useful for addressing the axion quality
problem. Rather, we rely on symmetries well motivated by other issues in BSM:
supersymmetry, $U(1)_{\rm B-L}$ and the discrete R-symmetry $Z_{NR}$. We show
that the interplay among these guarantees the high quality of the axion even
for the gravitino mass and axion decay constant as large as
$m_{3/2}=\mathcal{O}(10){\rm TeV}$ and $F_{a}=\mathcal{O}(10^{15}){\rm GeV}$
respectively. The key point of this work relies on the observation that the
MSSM contribution to the mixed anomalies $Z_{NR}-[SU(2)_{L}]^{2}$ and
$Z_{NR}-[SU(3)_{c}]^{2}$ is not enough for gauging $Z_{NR}$ for $N\neq6$, which
necessitates the introduction of new matter fields. We make the introduction to
achieve zero mixed anomalies, which logically supports a desired large enough
$N$ for $Z_{NR}$. This mechanism effectively makes $Z_{NR}$ equal to $U(1)_{R}$
and thus offers a logically complete solution to the axion quality problem.
