Is it time to go beyond $\Lambda$CDM universe?
  Concordance $\Lambda$CDM universe is the simplest model that is consistent
with a large variety of cosmological observations till date. But few recent
observations indicate inconsistencies in $\Lambda$CDM model. In this paper, we
consider the combination of recent SnIa+Bao+Cmb+Growth+$H(z)$+$H_{0}$
measurements to revisit the constraints on the dark energy evolution using the
widely studied CPL parametrisation for the dark energy equation of state.
Although the reconstructed behaviour for the dark energy equation of state
confirms the inconsistency of $\Lambda$CDM at $95\%$ confidence level, the
reconstructed $Om$ diagnostic which is a {\it null test} for $\Lambda$CDM,
still allows the concordance $\Lambda$CDM behaviour with a lower range of
$\Omega_{m0}$ than that obtained by Planck-2015. {\it This confirms that
$\Lambda$CDM is still the best choice for the dark energy model}. We also
measure the parameter $S = \sigma_{8}\sqrt{\Omega_{m0}/0.3} = 0.728 \pm 0.023$
which is consistent with its recent measurement by KiDS survey. The confidence
contour in the $\Omega_{m0}-\sigma_{8}$ parameter plane is also fully
consistent with KiDS survey measurement.
