The green bank telescope 350 Mhz drift-scan survey. I. survey observations and the discovery of 13 pulsars

J. Boyles, R. S. Lynch, S. M. Ransom, I. H. Stairs, D. R. Lorimer, M. A. McLaughlin, J. W.T. Hessels, V. M. Kaspi, V. I. Kondratiev, A. Archibald, A. Berndsen, R. F. Cardoso, A. Cherry, C. R. Epstein, C. Karako-Argaman, C. A. McPhee, T. Pennucci, M. S.E. Roberts, K. Stovall, J. Van Leeuwen

Research output: Contribution to journalArticlepeer-review

Abstract

Over the summer of 2007, we obtained 1191 hr of "drift-scan" pulsar search observations with the Green Bank Telescope at a radio frequency of 350 MHz. Here we describe the survey setup, search procedure, and the discovery and follow-up timing of 13 pulsars. Among the new discoveries, one (PSR J1623-0841) was discovered only through its single pulses, two (PSRs J1327-0755 and J1737-0814) are millisecond pulsars, and another (PSR J2222-0137) is a mildly recycled pulsar. PSR J1327-0755 is a 2.7 ms pulsar at a dispersion measure (DM) of 27.9 pc cm-3 in an 8.7 day orbit with a minimum companion mass of 0.22 Modot;. PSR J1737-0814 is a 4.2 ms pulsar at a DM of 55.3 pc cm-3 in a 79.3 day orbit with a minimum companion mass of 0.06 Modot;. PSR J2222-0137 is a 32.8 ms pulsar at a very low DM of 3.27 pc cm-3 in a 2.4 day orbit with a minimum companion mass of 1.11 Modot;. It is most likely a white-dwarf-neutron-star system or an unusual low-eccentricity double neutron star system. Ten other pulsars discovered in this survey are reported in the companion paper Lynch et al.

Original languageEnglish (US)
Article number80
JournalAstrophysical Journal
Volume763
Issue number2
DOIs
StatePublished - Feb 1 2013

Keywords

  • pulsars: general
  • pulsars: individual (PSR J1327-0755, PSR J1623-0841, PSR J1737-0814, PSR J1941-0121, PSR J2222-0137)
  • stars: neutron

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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