Papers › SPINN: a straightforward machine learning solution to the pulsar candidate selection problem

SPINN: a straightforward machine learning solution to the pulsar candidate selection problem

13 Jun 2014arXiv:1406.3627links table onlyarchive 2025-07-28

V. Morello, E. D. Barr, M. Bailes, C. M. Flynn, E. F. Keane, W. van Straten

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We describe SPINN (Straightforward Pulsar Identification using Neural Networks), a high-performance machine learning solution developed to process increasingly large data outputs from pulsar surveys. SPINN has been cross-validated on candidates from the southern High Time Resolution Universe (HTRU) survey and shown to identify every known pulsar found in the survey data while maintaining a false positive rate of 0.64%. Furthermore, it ranks 99% of pulsars among the top 0.11% of candidates, and 95% among the top 0.01%. In conjunction with the PEASOUP pipeline (Barr et al., in prep.), it has already discovered four new pulsars in a re-processing of the intermediate Galactic latitude area of HTRU, three of which have spin periods shorter than 5 milliseconds. SPINN's ability to reduce the amount of candidates to visually inspect by up to four orders of magnitude makes it a very promising tool for future large-scale pulsar surveys. In an effort to provide a common testing ground for pulsar candidate selection tools and stimulate interest in their development, we also make publicly available the set of candidates on which SPINN was cross-validated.

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as595/HTRU1 mentioned on GitHubpytorchGPL-3.0 report

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