The Parkes multibeam pulsar survey: VI. Discovery and timing of 142 pulsars and a Galactic population analysis

Abstract

[ABRIDGED] We present the discovery and follow-up observations of 142 pulsars found in the Parkes 20-cm multibeam pulsar survey of the Galactic plane. These new discoveries bring the total number of pulsars found by the survey to 742. In addition to tabulating spin and astrometric parameters, along with pulse width and flux density information, we present orbital characteristics for 13 binary pulsars which form part of the new sample. Combining these results from another recent Parkes multibeam survey at high Galactic latitudes, we have a sample of 1008 normal pulsars which we use to carry out a determination of their Galactic distribution and birth rate. We infer a total Galactic population of 30000 +/- 1100 potentially detectable pulsars (i.e. those beaming towards us) having 1.4-GHz luminosities above 0.1 mJy kpc squared. Using a pulsar current analysis, we derive the birth rate of this population to be 1.4 +/- 0.2 pulsars per century. An important conclusion from our work is that the inferred radial density function of pulsars depends strongly on the assumed distribution of free electrons in the Galaxy. As a result, any analyses using the most recent electron model of Cordes & Lazio predict a dearth of pulsars in the inner Galaxy. We show that this model can also bias the inferred pulsar scale height with respect to the Galactic plane. Combining our results with other Parkes multibeam surveys we find that the population is best described by an exponential distribution with a scale height of 330 pc.

30 pages, 8 figures, 9 tables, accepted for publication in MNRAS

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• Possible counterpart signal of the Fermi bubbles at the cosmic-ray positrons
• Pulsar Population Synthesis with Magnetorotational Evolution: Constraining the Decay of Magnetic field
• PSR J1227$-$6208 and its massive white dwarf companion: pulsar emission analysis, timing update and mass measurements
• Observations of the Fermi bubbles and the Galactic center excess with the DArk Matter Particle Explorer
• SPAN512: A new mid-latitude pulsar survey with the Nancay Radio Telescope
• Constraints on the origins of the Galactic neutrino flux
• Cosmic rays: interstellar gamma-ray and radio emission
• Magnetic braking of Ap/Bp stars: an alternative formation mechanism of compact intermediate-mass binary pulsars
• The Contribution From TeV Halos to the Isotropic Gamma-Ray Background
• Possible spectral irregularities in the AMS-02 positron spectrum
• Transient Radio Neutron Stars
• Microlensing pulsars
• Discovery of the anti-glitch in PSR J1835$-$1106
• Very high-energy gamma-ray and neutrino emission from hadronic interaction in compact binary millisecond pulsars
• Secular dynamics of the triple system harbouring PSR J0337+1715 and implications for the origin of its orbital configuration
• The traveling-PWN modeling attempt on the enigmatic LHAASO dumbbell-like structure
• Probing Galactic Diffuse TeV Gamma-Ray Emission with the HAWC Observatory
• First constraints on axion-like particles from Galactic sub-PeV gamma rays
• Main and interpulse interaction in PSRs J1842+0358 and J1926+0737: evidence for interpole communication
• Interpreting the LHAASO Galactic diffuse emission data
• Detectability of continuous gravitational waves from magnetically deformed neutron stars
• The Galactic population of canonical pulsars
• Pulsar-driven Jets in Supernovae, Gamma-Ray Bursts, and the Universe
• High Energy Radiation from Spider Pulsars
• A magnetospheric dichotomy for pulsars with extreme inclinations
• On the stochastic nature of Galactic cosmic-ray sources
• Common origin of the diffuse high energy backgrounds of gamma rays, neutrinos and cosmic ray positrons?
• Combined analyses of the antiproton production from cosmic-ray interactions and its possible dark matter origin
• Timing observations of three Galactic millisecond pulsars