21-cm foreground removal using AI and the frequency-difference technique
Creators
- 1. School of Aerospace Science and Technology, Xidian University, Xi'an 710126, People's Republic of China
- 2. Peng Cheng Laboratory, No. 2, Xingke 1st Street, Shenzhen 518000, People's Republic of China
- 3. School of Physics and Astronomy, Sun Yat-sen University, 2 Daxue Road, Tangjia, Zhuhai, 519082, People's Republic of China
- 4. CSST Science Center for the Guangdong-Hong Kong-Macau Greater Bay Area, Zhuhai 519082, People's Republic of China
- 5. Shanghai Astronomical Observatory (SHAO), Nandan Road 80, Shanghai 200030, China
- 6. University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China
- 7. National Key Laboratory of Radar Signal Processing, Xidian University, Xi'an 710126, People's Republic of China
Description
The deep learning technique has been employed in removing foreground contaminants from 21-cm intensity mapping, but its effectiveness is limited by the large dynamic range of the foreground amplitude. In this study, we develop a novel foreground removal technique grounded in U-Net networks. The essence of this technique lies in introducing an innovative data preprocessing step specifically, utilizing the temperature difference between neighboring frequency bands as input. Combining with the frequency difference, we refer to our method as the UNet-fd (UNet frequency-difference), where the U-Net structure is the same as that in deep21. Based on our tests, we demonstrate that this frequency-difference preprocessing technique can substantially reduce the dynamic range of foreground amplitudes by approximately two orders of magnitude. This reduction proves to be highly advantageous for the U-Net foreground removal. We observe that the HI signal can be reliably recovered, as indicated by the cross-correlation power spectra showing unity agreement at the scale of in the absence of instrumental effects. Moreover, accounting for the systematic beam effects, our reconstruction displays consistent autocorrelation and cross-correlation power spectrum ratios at the level across scales , with only a 10% reduction observed in the cross-correlation power spectrum at . The effects of redshift-space distortion are also reconstructed successfully, as evidenced by the quadrupole power spectra matching with the target truth. In order to test how thermal noise affects the performance of our method, we simulated various white noise levels in the map. This shows the mean cross-correlation ratio when the level of the thermal noise is smaller than or equal to that of the HI signal. In comparison, our method outperforms the traditional principal component analysis (PCA) method. The PCA-derived cross-correlation ratios are underestimated by around 60%. We conclude that the proposed frequency-difference technique can significantly enhance network performance by reducing the amplitude range of foregrounds and aiding in the prevention of HI loss.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.109.063509;
- arXiv
- arXiv:2310.06518;
- Crossref Funder ID
- 10.13039/501100012166; 10.13039/501100001809; 10.13039/501100012226; 10.13039/501100017596; 10.13039/501100021171; 10.13039/100018919; 10.13039/501100013314; 10.13039/501100005320; 10.13039/501100004921;
Publishing Information
- Journal Title
- Physical Review D
- Journal Volume
- 109
- Journal Issue
- 6
- Journal Page Range
- 19 pgs.
- ISSN
- 1089-4918
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S97: MATHEMATICAL METHODS AND COMPUTING;
- Descriptors DEI
- AMPLITUDES; APPROXIMATIONS; COMPARATIVE EVALUATIONS; CORRELATIONS; MACHINE LEARNING; MAPPING; NEURAL NETWORKS; NOISE; PERFORMANCE; PRINCIPAL COMPONENT ANALYSIS; RED SHIFT; REDUCTION; REMOVAL; SIGNAL-TO-NOISE RATIO; SIMULATION; SPECTRA
- Descriptors DEC
- ALGORITHMS; ARTIFICIAL INTELLIGENCE; CALCULATION METHODS; CHEMICAL REACTIONS; DIMENSIONLESS NUMBERS; EVALUATION; LEARNING; MATHEMATICAL LOGIC; MATHEMATICS; STATISTICS
Optional Information
- Copyright
- © 2024 American Physical Society
- Contract/Grant/Project number
- 2020YFC2201600; 12103037; 12203038; 11890691; XJS221312; 2022JQ-049; 2021A1515110057; B20019; 2022SKA0110200; 2022SKA0110202; 2020SKA0110402; 2020SKA0110401; CMS-CSST-2021 (A02, A03, B01)
- Notes
- Contact Email: fshi@xidian.edu.cn; Record automatically processed
- Funding organization
- National Key Research and Development Program of China; National Natural Science Foundation of China; Fundamental Research Funds for the Central Universities; Natural Science Basic Research Program of Shaanxi Province; Basic and Applied Basic Research Foundation of Guangdong Province; Peng Cheng Laboratory; Higher Education Discipline Innovation Project; Xidian University; Shanghai Jiao Tong University; National SKA Program of China; China Manned Space Project