Pulsar Candidate Sifting Using Multi-input Convolution Neural Networks. (arXiv:2007.14843v1 [astro-ph.IM])
<a href="http://arxiv.org/find/astro-ph/1/au:+Lin_H/0/1/0/all/0/1">Haitao Lin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Li_X/0/1/0/all/0/1">Xiangru Li</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zeng_Q/0/1/0/all/0/1">Qingguo Zeng</a>
Pulsar candidate sifting is an essential process for discovering new pulsars.
It aims to search for the most promising pulsar candidates from an all-sky
survey, such as High Time Resolution Universe (HTRU), Green Bank Northern
Celestial Cap (GBNCC), Five-hundred-meter Aperture Spherical radio Telescope
(FAST), etc. Recently, machine learning (ML) is a hot topic in pulsar candidate
sifting investigations. However, one typical challenge in ML for pulsar
candidate sifting comes from the learning difficulty arising from the highly
class-imbalance between the observation numbers of pulsars and non-pulsars.
Therefore, this work proposes a novel framework for candidate sifting, named
multi-input convolutional neural networks (MICNN). The MICNN is an architecture
of deep learning with four diagnostic plots of a pulsar candidate as its
inputs. To train our MICNN in a highly class-imbalanced dataset, a novel image
augment technique, as well as a three-stage training strategy, is proposed.
Experiments on observations from HTRU and GBNCC show the effectiveness and
robustness of these proposed techniques. In the experiments on HTRU, our MICNN
model achieves a recall of 0.962 and a precision rate of 0.967 even in a highly
class-imbalanced test dataset.
Pulsar candidate sifting is an essential process for discovering new pulsars.
It aims to search for the most promising pulsar candidates from an all-sky
survey, such as High Time Resolution Universe (HTRU), Green Bank Northern
Celestial Cap (GBNCC), Five-hundred-meter Aperture Spherical radio Telescope
(FAST), etc. Recently, machine learning (ML) is a hot topic in pulsar candidate
sifting investigations. However, one typical challenge in ML for pulsar
candidate sifting comes from the learning difficulty arising from the highly
class-imbalance between the observation numbers of pulsars and non-pulsars.
Therefore, this work proposes a novel framework for candidate sifting, named
multi-input convolutional neural networks (MICNN). The MICNN is an architecture
of deep learning with four diagnostic plots of a pulsar candidate as its
inputs. To train our MICNN in a highly class-imbalanced dataset, a novel image
augment technique, as well as a three-stage training strategy, is proposed.
Experiments on observations from HTRU and GBNCC show the effectiveness and
robustness of these proposed techniques. In the experiments on HTRU, our MICNN
model achieves a recall of 0.962 and a precision rate of 0.967 even in a highly
class-imbalanced test dataset.
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