Jason Boyles, Ryan Lynch, Scott M. Ransom, Ingrid H. Stairs, Duncan R. Lorimer, Maura A. McLaughlin, Jason W. T. Hessels, Vicky M. Kaspi, Vlad I. Kondratiev, Anne Archibald, Aaron Berndsen, Rogerio F. Cardoso, Angus Cherry, Christie A. McPhee, Tim Pennucci, Mallory S. E. Roberts, Kevin Stovall, Joeri van Leeuwen
Over the summer of 2007, we obtained 1191 hours 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 thirteen 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 DM of 27.9 pc cm^{-3} in a 8.7 day orbit with a minimum companion mass of 0.22$ solar mass. 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 solar mass. 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 solar mass. 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. 2012.
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http://arxiv.org/abs/1209.4293
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