  The latest Planck results reconfirm the existence of a slight but chronic
tension between the best-fit Cosmic Microwave Background (CMB) and low-redshift
observables: power seems to be consistently lacking in the late universe across
a range of observables (e.g.~weak lensing, cluster counts). We propose a
two-parameter model for dark energy where the dark energy is sufficiently like
dark matter at large scales to keep the CMB unchanged but where it does not
cluster at small scales, preventing concordance collapse and erasing power. We
thus exploit the generic scale-dependence of dark energy instead of the more
usual time-dependence to address the tension in the data. The combination of
CMB, distance and weak lensing data somewhat prefer our model to $\Lambda$CDM,
at $\Delta\chi^2=2.4$. Moreover, this improved solution has $\sigma_8=0.79 \pm
0.02$, consistent with the value implied by cluster counts.
