摘要: We present a method by using the phase characteristics of radio observation
data for pulsar search and candidate identification. The phase characteristics
are relations between the pulsar signal and the phase correction in the
frequency-domain, and we regard it as a new search diagnostic characteristic.
Based on the phase characteristics, a search method is presented: calculating
DM (dispersion measure) -- frequency data to select candidate frequencies, and
then confirming of candidates by using the broadband characteristics of pulsar
signals. Based on this method, we performed a search test on short observation
data of M15 and M71, which were observed by Five-hundred-meter Aperture
spherical radio Telescope (FAST), and some of the Galactic Plane Pulsar
Snapshot survey (GPPS) data. Results show that it can get similar search
results to PRESTO (PulsaR Exploration and Search TOolkit) while having a faster
processing speed.