2014MNRAS.443.1651M


Query : 2014MNRAS.443.1651M

2014MNRAS.443.1651M - Mon. Not. R. Astron. Soc., 443, 1651-1662 (2014/September-2)

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

MORELLO V., BARR E.D., BAILES M., FLYNN C.M., KEANE E.F. and VAN STRATEN W.

Abstract (from CDS):

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 per cent. Furthermore, it ranks 99 per cent of pulsars among the top 0.11 per cent of candidates, and 95 per cent among the top 0.01 per cent. In conjunction with the peasoup pipeline, 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 5ms. 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.

Abstract Copyright: © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2014)

Journal keyword(s): methods: data analysis - stars: neutron - pulsars: general

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 PSR J1017-7156 Psr 10 17 51.311783 -71 56 41.57398           ~ 61 1

Query : 2014MNRAS.443.1651M

Basic data :
PSR J1017-7156 -- Pulsar
Other object types:
otypes_help
Psr (PSR)
ICRS coord. (ep=J2000) :
10 17 51.311783 -71 56 41.57398 (Radio) [ 0.07675 0.06 90 ] B 2024MNRAS.530..287S
FK4 coord. (ep=B1950 eq=1950) :
10 16 45.823675 -71 41 38.35799 [ 0.07675 0.06 90 ]
Gal coord. (ep=J2000) :
291.558098233 -12.553267165 [ 0.07675 0.06 90 ]
Proper motions mas/yr :
-7.43 6.91 [0.08 0.07 90] C 2024MNRAS.530..287S
Parallaxes (mas):
1.5 [0.9] C 2024MNRAS.530..287S
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Identifiers (1) :
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PSR J1017-7156

References (61 between 1850 and 2026) (Total 61)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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