The Parkes Multibeam Pulsar Survey – II. Discovery and timing of 120 pulsars

By D. Morris, G. Hobbs, Andrew G. Lyne, Ingrid Stairs, F. Camilo, R. Manchester, A. Possenti, J. Bell, Victoria Kaspi, N. D. Amico and 3 more. 2002

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The Parkes Multibeam Pulsar Survey is a sensitive survey of a strip of the Galactic plane with |b| < 5 ◦ and 260 ◦ < l < 50 ◦ at 1374 MHz. Here we report the discovery of 120 new pulsars and subsequent timing observations, primarily using the 76-m Lovell radio telescope at Jodrell Bank. The main features of the sample of 370 published pulsars discovered during the multibeam survey are described. Furthermore, we highlight two pulsars: PSR J1734−3333, a young pulsar with the second highest surface magnetic field strength among the known radio pulsars, Bs = 5.4 × 10 13 G, and PSR J1830−1135, the second slowest radio pulsar known,

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/3cbdb26747cbf1195dca9470275efc907ea8678a

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Citations in the corpus

Pulsar Rotation Measures and the Large-Scale Structure of the Galactic Magnetic Field (2006, background): “The Parkes multibeam survey has discovered a large number of low-latitude and relatively distant pulsars (Manchester et al. 2001; Morris et al. 2002; Kramer et al. 2003; Hobbs et al. 2004), providing a unique opportunity to probe the diffuse magnetic field in a substantial fraction of the Galactic…”
Spectral properties of 441 radio pulsars (2017, methodology): “For PSR J1832–0644 the spectral index is determined from our data at 3.1 GHz and literature data at 1.4 GHz from PMPS (Morris et al. 2002) only.”
The Parkes multibeam pulsar survey – IV. Discovery of 180 pulsars and parameters for 281 previously known pulsars (2004, methodology): “Parameters for these pulsars were provided in Morris et al. (2002).”
Revisiting the radial distribution of pulsars in the Galaxy (2004, methodology): “The conclusion was the deficit of pulsars near the GC. Recent high frequency, sensitive Parkes Multibeam Pulsar Surveys (PMPS) (Manchester et al. 2001; Morris et al. 2002; Kramer et al. 2003) revealed many more distant pulsars with high Dispersion Measures (DM).”
A real-time fast radio burst: polarization detection and multiwavelength follow-up (2014, background): “FRB 140514 was discovered in a pointing centered just 9′ away from the nominal position of known FRB 110220 during a standard gridding (Morris et al. 2002) of the region in our survey.”
Physics of strongly magnetized neutron stars (2006, background): “…torques of a binary companion (Alpar et al 1982), and much lower surface magnetic fields in the range 108–1010 G. Recent surveys have also discovered pulsars with very high period derivatives (e.g. Morris et al (2002), McLaughlin et al (2003)) that imply surface fields up to around 1014 G.”
Pulsar nulling and mode changing (2007, unknown): “This long-period pulsar has a double-peaked mean profile of 50% width 98 ms or 0.034 in pulse phase (Morris et al. 2002).”
The Parkes Multibeam Pulsar Survey - III. Young Pulsars and the Discovery and Timing of 200 Pulsars (2003, background): “A detailed description of the survey including the motivation, telescope, hardware and software details, and the first 220 pulsars discovered were reported by Manchester et al. (2001) and Morris et al. (2002), hereafter Paper I and Paper II, respectively.”
The Parkes Multibeam Pulsar Survey - VI. Discovery and timing of 142 pulsars and a Galactic population analysis (2006, methodology): “Following the confirmation and positional refinement procedures described by Morris et al. (2002), each pulsar was observed regularly for at least one year using one or more of the Parkes, Lovell and Arecibo telescopes.”
Arecibo Pulsar Survey Using ALFA. I. Survey Strategy and First Discoveries (2005, background): “The Parkes multibeam (PMB) pulsar survey of the Galactic plane (Manchester et al. 2001; Morris et al. 2002; Kramer et al. 2003; Hobbs et al. 2004; Faulkner et al. 2004) has been extremely prolific, yielding over 700 new pulsars in the past seven years.”
Detection of 107 glitches in 36 southern pulsars (2012, background): “Since the end of the Multibeam Pulsar Survey timing (Morris et al. 2002), this source was not observed until the commencement of the Fermi project, leaving a data gap of ∼ 7 yr.”
The Parkes Multibeam Pulsar Survey - V. Finding binary and millisecond pulsars (2004, background): “It has been very successful, with reported discoveries of more than 600 new pulsars so far, discussed in Paper I, Morris et al. (2002), Kramer et al. (2003) and Hobbs et al. (2004).”