  Rotating radio transients (RRATs) are neutron stars that emit detectable
radio bursts sporadically. They are statistically distinct in the neutron star
population, in many observable properties, but by their nature are practically
difficult to study in depth. In this paper, we present the results from 1408 h
of observations of RRAT candidates using the Irish station of the Low Frequency
Array (LOFAR) at 150 MHz. As of October 2022, this census involved observing
113 sources, leading to 29 detections which were then followed up
systematically. Single-pulse emission was detected from 25 sources, and
periodic emission from 14 sources. 18 sources were found to have emission
behaviour that is not discussed in prior works using LOFAR instruments. Four
novel or modified source periods have been determined, ranging from 1.5-3.9 s,
and 8 new or updated phase-coherent pulsar timing ephemerides have been
produced using detected bursts. One unexpected single-pulse with a
clearly-Galactic dispersion measure was detected as a part of this work, but
has not been re-detected in follow-up observations. Observations are ongoing to
expand the number of observed sources and further characterise and improve
ephemerides for the detected sources. This census has demonstrated the
capability for international LOFAR stations to detect, monitor and characterise
a significant fraction of these unique sources.
