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Title:
Discovery of three new pulsars in a 610-MHz pulsar survey with the GMRT
Authors:
Joshi, B. C.; McLaughlin, M. A.; Lyne, A. G.; Ludovici, D. A.; Pawar, N. A.; Faulkner, A. J.; Lorimer, D. R.; Kramer, M.; Davies, M. L.
Affiliation:
AA(National Centre for Radio Astrophysics, Post Bag 3, Ganeshkhind, Pune 411 007, India), AB(Department of Physics, West Virginia University, 210 Hodges Hall, Morgantown, WV 26506, USA), AC(Jodrell Bank Centre for Astrophysics, University of Manchester, Alan-Turing Building, Oxford Road, Manchester M13 9PL), AD(Department of Physics, West Virginia University, 210 Hodges Hall, Morgantown, WV 26506, USA), AE(National Centre for Radio Astrophysics, Post Bag 3, Ganeshkhind, Pune 411 007, India), AF(Jodrell Bank Centre for Astrophysics, University of Manchester, Alan-Turing Building, Oxford Road, Manchester M13 9PL; Astrophysics Group, University of Cambridge, Cavendish Laboratory, J J Thomson Avenue, Cambridge CB3 0HE), AG(Department of Physics, West Virginia University, 210 Hodges Hall, Morgantown, WV 26506, USA), AH(Jodrell Bank Centre for Astrophysics, University of Manchester, Alan-Turing Building, Oxford Road, Manchester M13 9PL; MPI fuer Radioastronomie, Auf dem Huegel 69, 53121 Bonn, Germany), AI(Astrophysics Group, University of Cambridge, Cavendish Laboratory, J J Thomson Avenue, Cambridge CB3 0HE)
Publication:
Monthly Notices of the Royal Astronomical Society, Volume 398, Issue 2, pp. 943-948. (MNRAS Homepage)
Publication Date:
09/2009
Origin:
MNRAS
MNRAS Keywords:
stars: neutron , pulsars: general , pulsars: individual: J0026+6320 , pulsars: individual: J2208+5500 , pulsars: individual: J2217+5733
DOI:
10.1111/j.1365-2966.2009.15125.x
Bibliographic Code:
2009MNRAS.398..943J

Abstract

We report on the discovery of three new pulsars in the first blind survey of the north Galactic plane (45° < l < 135° |b| < 1°) with the Giant Meterwave Radio telescope (GMRT) at an intermediate frequency of 610 MHz. The survey covered 106 deg2 with a sensitivity of roughly 1 mJy to long-period pulsars (pulsars with period longer than 1 s). The three new pulsars have periods of 318, 933 and 1056 ms. Their timing parameters and flux densities, obtained in follow-up observations with the Lovell Telescope at Jodrell Bank and the GMRT, are presented. We also report on pulse nulling behaviour in one of the newly discovered pulsars, PSR J2208+5500.
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