A newly-discovered pulsar at high Galactic latitude displays both bright, sporadic, variable bursts characteristic of Rotating Radio Transients, and a dim, relatively stable pulse component that is typical of canonical pulsars. This makes it part of a small but growing group of objects that may be "missing links" between the two populations. We propose two 8-hour observations to properly time the pulsar in order to better constrain its magnetic field and characteristic age, and to build up a more complete sample of its pulse fluences, that would then enable comparisons between this source and other pulsars.