The Green Bank North Celestial Cap Pulsar Survey. IV. Four New Timing Solutions

R. J. Aloisi, A. Cruz, L. Daniels, N. Meyers, R. Roekle, A. Schuett, J. K. Swiggum, M. E. Decesar, D. L. Kaplan, R. S. Lynch, K. Stovall, Lina Levin, A. M. Archibald, S. Banaszak, C. M. Biwer, J. Boyles, P. Chawla, L. P. Dartez, B. Cui, D. F. DayA. J. Ford, J. Flanigan, E. Fonseca, J. W.T. Hessels, J. Hinojosa, C. Karako-Argaman, V. M. Kaspi, V. I. Kondratiev, S. Leake, G. Lunsford, J. G. Martinez, A. Mata, M. A. Mclaughlin, H. Al Noori, S. M. Ransom, M. S.E. Roberts, M. D. Rohr, X. Siemens, R. Spiewak, I. H. Stairs, J. Van Leeuwen, A. N. Walker, B. L. Wells

Research output: Contribution to journalArticlepeer-review


We present timing solutions for four pulsars discovered in the Green Bank Northern Celestial Cap survey. All four pulsars are isolated with spin periods between 0.26 and 1.84 s. PSR J0038-2501 has a 0.26 s period and a period derivative of 7.6 × 10-19 s s-1, which is unusually low for isolated pulsars with similar periods. This low period derivative may be simply an extreme value for an isolated pulsar or it could indicate an unusual evolution path for PSR J0038-2501, such as a disrupted recycled pulsar from a binary system or an orphaned central compact object (CCO). Correcting the observed spin-down rate for the Shklovskii effect suggests that this pulsar may have an unusually low space velocity, which is consistent with expectations for DRPs. There is no X-ray emission detected from PSR J0038-2501 in an archival Swift observation, which suggests that it is not a young orphaned CCO. The high dispersion measure of PSR J1949+3426 suggests a distance of 12.3 kpc. This distance indicates that PSR J1949+3426 is among the most distant 7% of Galactic field pulsars, and is one of the most luminous pulsars.

Original languageEnglish (US)
Article number19
JournalAstrophysical Journal
Issue number1
StatePublished - Apr 10 2019

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science


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