  We present Clusterrank, a new algorithm for identifying dispersed
astrophysical pulses. Such pulses are commonly detected from Galactic pulsars
and rotating radio transients (RRATs), which are neutron stars with sporadic
radio emission. More recently, isolated, highly dispersed pulses dubbed fast
radio bursts (FRBs) have been identified as the potential signature of an
extragalactic cataclysmic radio source distinct from pulsars and RRATs.
Clusterrank helped us discover 14 pulsars and 8 RRATs in data from the Arecibo
327 MHz Drift Pulsar Survey (AO327). The new RRATs have DMs in the range $23.5
- 86.6$ pc cm$^{-3}$ and periods in the range $0.172 - 3.901$ s. The new
pulsars have DMs in the range $23.6 - 133.3$ pc cm$^{-3}$ and periods in the
range $1.249 - 5.012$ s, and include two nullers and a mode-switching object.
We estimate an upper limit on the all-sky FRB rate of $10^5$ day$^{-1}$ for
bursts with a width of 10 ms and flux density $\gtrsim 83$ mJy. The DMs of all
new discoveries are consistent with a Galactic origin. In comparing statistics
of the new RRATs with sources from the RRATalog, we find that both sets are
drawn from the same period distribution. In contrast, we find that the period
distribution of the new pulsars is different from the period distributions of
canonical pulsars in the ATNF catalog or pulsars found in AO327 data by a
periodicity search. This indicates that Clusterrank is a powerful complement to
periodicity searches and uncovers a subset of the pulsar population that has so
far been underrepresented in survey results and therefore in Galactic pulsar
population models.

High Energy Astrophysical Phenomena;Instrumentation and Methods for Astrophysics;Solar and Stellar Astrophysics