Study of 72 Pulsars Discovered in the PALFA Survey: Timing Analysis, Glitch Activity, Emission Variability, and a Pulsar in an Eccentric Binary

@article{Parent2022StudyO7,
  title={Study of 72 Pulsars Discovered in the PALFA Survey: Timing Analysis, Glitch Activity, Emission Variability, and a Pulsar in an Eccentric Binary},
  author={E. Parent and H. Sewalls and Paulo C. C. Freire and T. Matheny and Andrew G. Lyne and Benetge B. P. Perera and F. Cardoso and Maura Mclaughlin and Bruce Allen and Adam Brazier and Fernando Camilo and Shami Chatterjee and James M. Cordes and Fronefield Crawford and Julia S. Deneva and F. A. Dong and Robert D. Ferdman and Emmanuel Fonseca and Jason W. T. Hessels and Victoria M. Kaspi and Benjamin Knispel and Joeri van Leeuwen and Ryan S. Lynch and B. M. Meyers and James W. McKee and M. B. Mickaliger and Chitrang Patel and Scott M. Ransom and Andr{\'e} Rochon and Paul Scholz and Ingrid H. Stairs and Ben W. Stappers and C. M. Tan and W. W. Zhu},
  journal={The Astrophysical Journal},
  year={2022},
  volume={924}
}
We present new discoveries and results from long-term timing of 72 pulsars discovered in the Pulsar Arecibo L-band Feed Array (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, 12 nulling and two intermittent pulsars. We detected eight glitches in five… 

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