  It has been recently suggested~\cite{Berezhiani:2015yta} that a subdominant
fraction of dark matter decaying after recombination may alleviate tension
between high-redshift (CMB anisotropy) and low-redshift (Hubble constant,
cluster counts) measurements. In this report, we continue our previous
study~\cite{Chudaykin:2016yfk} of the decaying dark matter (DDM) model adding
all available recent baryon acoustic oscillation (BAO) and redshift space
distortions (RSD) measurements. We find, that the BAO/RSD measurements
generically prefer the standard $\Lambda$CDM and combined with other
cosmological measurements impose an upper limit on the DDM fraction at the
level of $\sim$\,5\,\%, strengthening by a factor of 1.5 limits obtained in
\cite{Chudaykin:2016yfk} mostly from CMB data. However, the numbers vary from
one analysis to other based on the same Baryon Oscillation Spectroscopic Survey
(BOSS) Data Release 12 (DR12) galaxy sample. Overall, the model with a few
percent DDM fraction provides a better fit to the combined cosmological data as
compared to the $\Lambda$CDM: the cluster counting and direct measurements of
the Hubble parameter are responsible for that. The improvement can be as large
as 1.5\,$\sigma$ and grows to 3.3\,$\sigma$ when the CMB lensing power
amplitude ${\rm
  A_L}$ is introduced as a free fitting parameter.
