  A search for pulsed radiation at a frequency of 111 MHz in the direction of
116 RRAT candidates was carried out. For the search, archival data obtained on
a meridian 128-beam radio telescope, a Large Phased Array (LPA), was used. For
each candidate, about six days of observations were accumulated over an
interval of eight years. Eleven new RRATs have been discovered. It was possible
to estimate periods for six of them, and to construct average profiles for four
of them. Some of the candidates turned out to be known pulsars observed in the
side lobes of the radio telescope and interference. For the part of the
candidates could not find pulses with a signal-to-noise ratio of more than
seven, and their nature remains unknown.
