  We report on the results of a search for radio pulsars in five supernova
remnants (SNRs) with FAST. The observations were made using the 19-beam
receiver in the Snapshot mode. The integration time for each pointing is 10
min. We discovered a new pulsar PSR J1845$-$0306 which has a spin period of
983.6 ms and a dispersion measure of 444.6$\pm$2.0 cm$^{-3}$ pc in observations
of SNR G29.6+0.1. To judge the association between the pulsar and the SNR,
further verification is needed. We also re-detected some known pulsars in the
data from SNRs G29.6+0.1 and G29.7$-$0.3. No pulsars were detected in
observations of other three SNRs.
