  We measure the cross-power spectrum between galaxy density from
Canada-France-Hawaii-Telescope Lensing Survey (CFHTLenS) catalogues and
gravitational lensing convergence from Planck data release 1 (2013) and 2
(2015). We investigate three main galaxy samples: $18.0<i_{\rm AB}<22.0$,
$18.0<i_{\rm AB}<23.0$, $18.0<i_{\rm AB}<24.0$ in the redshift range
$0.2<z<1.3$ in each of the four CFHTLenS wide fields. By comparing the measured
cross-spectrum with model predictions, linear galaxy-dark matter biases of
$b=0.82^{+0.24}_{-0.23}, 0.83^{+0.19}_{-0.18}, 0.82^{+0.16}_{-0.14}$ are
inferred at significances of $3.5, 4.5, 5.6\sigma$ using the Planck 2015
release. These measurements are marginally consistent with biases derived from
galaxy-galaxy auto-correlations: $b=1.15^{+0.02}_{-0.01}, 1.08^{+0.01}_{-0.01}$
and $0.96^{+0.01}_{-0.01}$ respectively. Using the 2013 Planck release, we
obtain biases of $b=1.33^{+0.29}_{-0.28}, 1.19^{+0.23}_{-0.23},
1.16^{+0.19}_{-0.18}$, showing significant differences between the releases.
