  In a systematic program to characterise the intra-night optical variability
(INOV) of different classes of narrow-line Seyfert 1 galaxies (NLSy1s), we
report here the first comparative INOV study of NLSy1 sets detected in the
X-ray and $\gamma$-ray bands. Our sample consists of 18 sources detected in
X-ray but not in $\gamma$-rays (hereafter x$\textunderscore$NLSy1s) and 7
sources detected in $\gamma$-rays (hereafter g$\textunderscore$NLSy1s), out of
which 5 are detected also in X-rays. We have monitored these two sets of
NLSy1s, respectively, in 24 and 21 sessions of a minimum of 3 hours duration
each. The INOV duty cycles for these two sets are found to be 12\% and 53\%,
respectively (at a 99\% confidence level). In the set of 18
x$\textunderscore$NLSy1s, INOV duty cycle is found to be zero for the 13
radio-quiet members (monitored in 14 sessions) and 43\% for the 5 radio-loud
members (10 sessions). The latter is very similar to the aforementioned duty
cycle of 53\% found here for the set of g$\textunderscore$NLSy1s (all of which
are radio-loud). Thus it appears that the radio loudness level is the prime
factor behind the INOV detection and the pattern of the high-energy radiation
plays only a minor role.
