2014ApJ...781..117Z


Query : 2014ApJ...781..117Z

2014ApJ...781..117Z - Astrophys. J., 781, 117 (2014/February-1)

Searching for pulsars using image pattern recognition.

ZHU W.W., BERNDSEN A., MADSEN E.C., TAN M., STAIRS I.H., BRAZIER A., LAZARUS P., LYNCH R., SCHOLZ P., STOVALL K., RANSOM S.M., BANASZAK S., BIWER C.M., COHEN S., DARTEZ L.P., FLANIGAN J., LUNSFORD G., MARTINEZ J.G., MATA A., ROHR M., WALKER A., ALLEN B., BHAT N.D.R., BOGDANOV S., CAMILO F., CHATTERJEE S., CORDES J.M., CRAWFORD F., DENEVA J.S., DESVIGNES G., FERDMAN R.D., FREIRE P.C.C., HESSELS J.W.T., JENET F.A., KAPLAN D.L., KASPI V.M., KNISPEL B., LEE K.J., VAN LEEUWEN J., LYNE A.G., McLAUGHLIN M.A., SIEMENS X., SPITLER L.G. and VENKATARAMAN A.

Abstract (from CDS):

In the modern era of big data, many fields of astronomy are generating huge volumes of data, the analysis of which can sometimes be the limiting factor in research. Fortunately, computer scientists have developed powerful data-mining techniques that can be applied to various fields. In this paper, we present a novel artificial intelligence (AI) program that identifies pulsars from recent surveys by using image pattern recognition with deep neural nets–the PICS (Pulsar Image-based Classification System) AI. The AI mimics human experts and distinguishes pulsars from noise and interference by looking for patterns from candidate plots. Different from other pulsar selection programs that search for expected patterns, the PICS AI is taught the salient features of different pulsars from a set of human-labeled candidates through machine learning. The training candidates are collected from the Pulsar Arecibo L-band Feed Array (PALFA) survey. The information from each pulsar candidate is synthesized in four diagnostic plots, which consist of image data with up to thousands of pixels. The AI takes these data from each candidate as its input and uses thousands of such candidates to train its ∼9000 neurons. The deep neural networks in this AI system grant it superior ability to recognize various types of pulsars as well as their harmonic signals. The trained AI's performance has been validated with a large set of candidates from a different pulsar survey, the Green Bank North Celestial Cap survey. In this completely independent test, the PICS ranked 264 out of 277 pulsar-related candidates, including all 56 previously known pulsars and 208 of their harmonics, in the top 961 (1%) of 90,008 test candidates, missing only 13 harmonics. The first non-pulsar candidate appears at rank 187, following 45 pulsars and 141 harmonics. In other words, 100% of the pulsars were ranked in the top 1% of all candidates, while 80% were ranked higher than any noise or interference. The performance of this system can be improved over time as more training data are accumulated. This AI system has been integrated into the PALFA survey pipeline and has discovered six new pulsars to date.

Abstract Copyright: ∼

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

Simbad objects: 6

goto Full paper

goto View the references in ADS

Number of rows : 6
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 J1854+00 Psr 18 54 43.59750 +00 51 09.5007           ~ 4 0
2 PSR J1901+02 Psr 19 01 +02.0           ~ 2 0
3 PSR J1903+04 Psr 19 03 +04.0           ~ 2 0
4 PSR J1914+08 Psr 19 14 06.51610 +08 41 40.0949           ~ 4 0
5 PSR J1930+17 Psr 19 30 44 +17 25.0           ~ 6 0
6 PSR J1938+20 Psr 19 38 12 +20 10.0           ~ 2 0

To bookmark this query, right click on this link: simbad:objects in 2014ApJ...781..117Z and select 'bookmark this link' or equivalent in the popup menu