  The International Pulsar Timing Array 2nd data release is the combination of
datasets from worldwide collaborations. In this study, we search for continuous
waves: gravitational wave signals produced by individual supermassive black
hole binaries in the local universe. We consider binaries on circular orbits
and neglect the evolution of orbital frequency over the observational span. We
find no evidence for such signals and set sky averaged 95% upper limits on
their amplitude h 95 . The most sensitive frequency is 10nHz with h 95 = 9.1
10-15 . We achieved the best upper limit to date at low and high frequencies of
the PTA band thanks to improved effective cadence of observations. In our
analysis, we have taken into account the recently discovered common red noise
process, which has an impact at low frequencies. We also find that the peculiar
noise features present in some pulsars data must be taken into account to
reduce the false alarm. We show that using custom noise models is essential in
searching for continuous gravitational wave signals and setting the upper
limit.
