creased to avoid structural information loss, this graph
kernel is no longer efficient. Hence, MDKV repre-
sents star structures of height greater than one as vec-
tors and sums their Euclidean distances. It runs in
O(h(υ
3
+|Σ|υ
2
)), where Σ is a set of vertexlabels and
graphs are iteratively relabeled h times. We verified
the computational efficiency of the proposed graph
kernels on artificially generated datasets. Further, re-
sults on three real-world datasets showedthat the clas-
sification accuracy of the proposed graph kernels is
higher than three conventional graph kernel methods.
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