  We report new high-quality galaxy scale strong lens candidates found in the
Kilo Degree Survey data release 4 using Machine Learning. We have developed a
new Convolutional Neural Network (CNN) classifier to search for gravitational
arcs, following the prescription by \cite{2019MNRAS.484.3879P} and using only
$r-$band images. We have applied the CNN to two "predictive samples": a
Luminous red galaxy (LRG) and a "bright galaxy" (BG) sample ($r<21$). We have
found 286 new high probability candidates, 133 from the LRG sample and 153 from
the BG sample. We have then ranked these candidates based on a value that
combines the CNN likelihood to be a lens and the human score resulting from
visual inspection (P-value) and we present here the highest 82 ranked
candidates with P-values $\ge 0.5$. All these high-quality candidates have
obvious arc or point-like features around the central red defector. Moreover,
we define the best 26 objects, all with scores P-values $\ge 0.7$ as a "golden
sample" of candidates. This sample is expected to contain very few false
positives and thus it is suitable for follow-up observations. The new lens
candidates come partially from the the more extended footprint adopted here
with respect to the previous analyses, partially from a larger predictive
sample (also including the BG sample). These results show that machine learning
tools are very promising to find strong lenses in large surveys and more
candidates that can be found by enlarging the predictive samples beyond the
standard assumption of LRGs. In the future, we plan to apply our CNN to the
data from next-generation surveys such as the Large Synoptic Survey Telescope,
Euclid, and the Chinese Space Station Optical Survey.
