Discovery of 72 pulsars in the PALFA survey: Timing analysis, glitch activity, emission variability, and a pulsar in an eccentric binary

We present results from long-term timing of 72 pulsars discovered by the Arecibo PALFA survey, including precise determination of astrometric and spin parameters, and flux density and scatter broadening measurements at 1.4 GHz. Notable discoveries include two young pulsars (characteristic ages ∼30 kyr) with no apparent supernova remnant associations, three mode changing, 13 nulling and two intermittent pulsars. We detected eight glitches in five pulsars. Among them is PSR J1939+2609, an apparently old pulsar (characteristic age ∼1 Gy), and PSR J1954+2529, which likely belongs to a newly-emerging class of binary pulsars. The latter is the only pulsar among the 72 that appears to be not isolated: a non-recycled neutron star with a 931 ms spin period in an eccentric (e = 0.114) wide (Pb = 82.7 d) orbit with a companion of undetermined nature having a minimum mass of 0.61M . Since operations at Arecibo ceased in 2020 August, we give a final tally of PALFA sky coverage, and compare its 207 pulsar discoveries to the known population. On average, they are 50% more distant than other Galactic plane radio pulsars; PALFA millisecond pulsars (MSP) have twice the dispersion Corresponding author: E. Parent parente@physics.mcgill.ca ar X iv :2 10 8. 02 32 0v 2 [ as tr oph .H E ] 6 A ug 2 02 1