Deep learning approach for identification of H II regions during reionization in 21-cm observations

被引:30
作者
Bianco, Michele [1 ,2 ]
Giri, Sambit K. [2 ,3 ]
Iliev, Ilian T. [1 ]
Mellema, Garrelt [2 ]
机构
[1] Univ Sussex, Astron Ctr, Dept Phys & Astron, Pevensey 3 Bldg, Brighton BN1 9QH, E Sussex, England
[2] Stockholm Univ, Oskar Klein Ctr, Dept Astron, AlbaNova, SE-10691 Stockholm, Sweden
[3] Univ Zurich, Inst Computat Sci, Winterthurerstr 190, CH-8057 Zurich, Switzerland
基金
英国科学技术设施理事会; 瑞典研究理事会;
关键词
image processing; interferometric; dark ages; reionization; first stars; early Universe; APPROXIMATE-TO; 9.1; 21 CM SIGNAL; INTERGALACTIC MEDIUM; COSMIC REIONIZATION; NEUTRAL HYDROGEN; IONIZED BUBBLES; SIZE STATISTICS; EPOCH; SIMULATIONS; CONSTRAINTS;
D O I
10.1093/mnras/stab1518
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The upcoming Square Kilometre Array (SKA-Low) will map the distribution of neutral hydrogen during reionization and produce a tremendous amount of three-dimensional tomographic data. These image cubes will be subject to instrumental limitations, such as noise and limited resolution. Here, we present SegU-Net, a stable and reliable method for identifying neutral and ionized regions in these images. SegU-Net is a U-Net architecture-based convolutional neural network for image segmentation. It is capable of segmenting our image data into meaningful features (ionized and neutral regions) with greater accuracy compared to previous methods. We can estimate the ionization history from our mock observation of SKA with an observation time of 1000 h with more than 87 percent accuracy. We also show that SegU-Net can be used to recover the size distributions and Betti numbers, with a relative difference of only a few percent from the values derived from the original smoothed and then binarized neutral fraction field. These summary statistics characterize the non-Gaussian nature of the reionization process.
引用
收藏
页码:3982 / 3997
页数:16
相关论文
共 119 条
[1]   SLIC Superpixels Compared to State-of-the-Art Superpixel Methods [J].
Achanta, Radhakrishna ;
Shaji, Appu ;
Smith, Kevin ;
Lucchi, Aurelien ;
Fua, Pascal ;
Suesstrunk, Sabine .
IEEE TRANSACTIONS ON PATTERN ANALYSIS AND MACHINE INTELLIGENCE, 2012, 34 (11) :2274-2281
[2]  
Aghanim N., 2020, ASTRON ASTROPHYS, V641, pA6, DOI DOI 10.1051/0004-6361/201833910
[3]   Non-linear bias of cosmological halo formation in the early universe [J].
Ahn, Kyungjin ;
Iliev, Ilian T. ;
Shapiro, Paul R. ;
Srisawat, Chaichalit .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2015, 450 (02) :1486-1502
[4]  
[Anonymous], 2017, ARXIV170605721
[5]  
[Anonymous], 2014, CORR
[6]  
[Anonymous], 2017, arXiv
[7]  
[Anonymous], 2015, Proc. Sci. The Cosmic Dawn and Epoch of Reionization withthe Square Kilometre Array
[8]  
[Anonymous], 2018, A guide to convolution arithmetic for deep learning
[9]  
[Anonymous], 2012, ARXIV PREPRINT ARXIV
[10]  
Betti E., 1870, Ann. Mat. Pura Appl., V4, P140