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The High Time Resolution Universe Pulsar Survey - VI. An artificial neural network and timing of 75 pulsars

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posted on 2024-08-06, 09:34 authored by S. D. Bates, Matthew BailesMatthew Bailes, B. R. Barsdell, N. D. R. Bhat, M. Burgay, S. Burke-Spolaor, D. J. Champion, P. Coster, N. D'Amico, A. Jameson, S. Johnston, M. J. Keith, M. Kramer, L. Levin, A. Lyne, S. Milia, C. Ng, C. Nietner, A. Possenti, B. Stappers, D. Thornton, Willem van Straten
We present 75 pulsars discovered in the mid-latitude portion of the High Time Resolution Universe survey, 54 of which have full timing solutions. All the pulsars have spin periods greater than 100ms, and none of those with timing solutions is in binaries. Two display particularly interesting behaviour; PSR J1054-5944 is found to be an intermittent pulsar, and PSR J1809-0119 has glitched twice since its discovery. In the second half of the paper we discuss the development and application of an artificial neural network in the data-processing pipeline for the survey. We discuss the tests that were used to generate scores and find that our neural network was able to reject over 99per cent of the candidates produced in the data processing, and able to blindly detect 85per cent of pulsars. We suggest that improvements to the accuracy should be possible if further care is taken when training an artificial neural network; for example, ensuring that a representative sample of the pulsar population is used during the training process, or the use of different artificial neural networks for the detection of different types of pulsars.

Funding

Science and Technology Facilities Council

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ISSN

0035-8711

Journal title

Monthly Notices of the Royal Astronomical Society

Volume

427

Issue

2

Pagination

13 pp

Publisher

Wiley

Copyright statement

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2012 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

Language

eng

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