Characterization of inpaint residuals in interferometric measurements of the epoch of reionization
Characterization of inpaint residuals in interferometric measurements of the epoch of reionization
复制标题
再电离时代干涉测量中修复残差的表征
DOI:
10.1093/mnras/stad441
复制
发表时间:
2023
影响因子:
4.8
通讯作者:
Adams, Tyrone
中科院分区:
文献类型:
--
作者:
Pagano, Michael;Liu, Jing;Liu, Adrian;Kern, Nicholas S;Ewall-Wice, Aaron;Bull, Philip;Pascua, Robert;Ravanbakhsh, Siamak;Abdurashidova, Zara;Adams, Tyrone
To mitigate the effects of Radio Frequency Interference (RFI) on the data analysis pipelines of 21 cm interferometric instruments, numerous inpaint techniques have been developed. In this paper, we examine the qualitative and quantitative errors introduced into the visibilities and power spectrum due to inpainting. We perform our analysis on simulated data as well as real data from the Hydrogen Epoch of Reionization Array (HERA) Phase 1 upper limits. We also introduce a convolutional neural network that is capable of inpainting RFI corrupted data. We train our network on simulated data and show that our network is capable of inpainting real data without requiring to be retrained. We find that techniques that incorporate high wavenumbers in delay space in their modelling are best suited for inpainting over narrowband RFI. We show that with our fiducial parameters discrete prolate spheroidal sequences (dpss) andcleanprovide the best performance for intermittent RFI while Gaussian progress regression (gpr) and least squares spectral analysis (lssa) provide the best performance for larger RFI gaps. However, we caution that these qualitative conclusions are sensitive to the chosen hyperparameters of each inpainting technique. We show that all inpainting techniques reliably reproduce foreground dominated modes in the power spectrum. Since the inpainting techniques should not be capable of reproducing noise realizations, we find that the largest errors occur in the noise dominated delay modes. We show that as the noise level of the data comes down,cleananddpssare most capable of reproducing the fine frequency structure in the visibilities.