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.

Deep learning approach for identification of H ii regions during reionization in 21-cm observations – II. Foreground contamination

Mesinger, Andrei;
2024

Abstract

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.
2024
Settore FIS/05 - Astronomia e Astrofisica
Dark ages; reionization; first stars; early Universe; techniques: image processing; techniques: interferometric; approximate-to 9.1; 21 cm signal; intergalactic medium; neutral hydrogen; ionized bubbles; size statistics; epoch; simulations; constraints
   University of Sussex Astronomy Consolidated Grant 2020-2023
   UK Research and Innovation
   STFC
   ST/T000473/1

   University of Sussex Astronomy Consolidated Grant 2020-2023
   UK Research and Innovation
   STFC
   ST/T000473/1

   Astrophysics and Cosmology at the University of Sussex (2011-2016)
   UK Research and Innovation
   STFC
   ST/I000976/1
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11384/139783
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