Translator Disclaimer
Poster + Paper
13 December 2020 Identification of infrared-ring structures by convolutional neural network
Author Affiliations +
Conference Poster
Recently, the amount of data obtained from astronomical instruments has been increasing explosively, and data science methods such as Machine Learning/Deep Learning gain attention on the back of the growth in demand for automatic analysis. Using these methods, the number of applications to the target sources that have clear boundaries with the background i.e., stars, planets, and galaxies is increasing year by year. However, there are a few studies which applied the data science methods to the interstellar medium (ISM) distributed in the Galactic plane, which have complicated and ambiguous silhouettes. We aim to develop classifiers to automatically extract various structures of the ISM by Convolutional Neural Network (CNN) that is strong in image recognition even in deep learning. In this study, we focus on the infra-red (IR) ring structures distributed in the Galactic plane. Based on the catalog of Churchwell et al. (2006, 2007), we created a “Ring” dataset from the Spitzer/GLIMPSE 8 μm and Spitzer/MIPSGAL 24 μm data and optimized the parameters of the CNN model. We applied the developed model to a range of 16.5° ≤ l ≤ 19.5°, |b| ≤ 1° . As a result, 234 “Ring” candidates are detected. The “Ring” candidates were matched with 75% Milky Way Project (MWP, Simpson et al. 2012) “Ring” and 65% WISE Hii region catalog (Anderson et al. 2014). In addition, new“Ring”and Hii region candidate objects were also found. For these results, we conclude that the CNN model may have a recognition accuracy equal to or better than that of human eyes.
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Shota Ueda, Shinji Fujita, Atsushi Nishimura, Toshikazu Onishi, Yoshito Shimajiri, Yusuke Miyamoto, Kazufumi Torii, Atsushi M. Ito, Shunya Takekawa, Hiroyuki Kaneko, Daisuke Yoshida, Taro Matsuo, Tsuyoshi Inoue, Yasutomo Kawanishi, and Kazuki Tokuda "Identification of infrared-ring structures by convolutional neural network", Proc. SPIE 11452, Software and Cyberinfrastructure for Astronomy VI, 114522L (13 December 2020);


Fluid mechanics leads to life in the universe
Proceedings of SPIE (October 15 2012)
Objectives for the Space Infrared Telescope Facility
Proceedings of SPIE (December 01 1991)
The next-generation infrared space telescope SPICA
Proceedings of SPIE (September 21 2012)
Recent Results From The UKIRT Infrared Camera, IRCAM
Proceedings of SPIE (September 26 1989)

Back to Top