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FF vs ¯ í µí±¥ HI plots are shown for the data cubes of 600 3 grid units and 300 3 grid units. It can be seen that the time evolution for Filling Factor (FF) remains unchanged even after the resolution of the maps are lowered and the mean is subtracted.

FF vs ¯ í µí±¥ HI plots are shown for the data cubes of 600 3 grid units and 300 3 grid units. It can be seen that the time evolution for Filling Factor (FF) remains unchanged even after the resolution of the maps are lowered and the mean is subtracted.

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Figure 2. FF vs ¯ í µí±¥ HI plots are shown for the data cubes of 600 3...
Figure 3. Pictorial representation of the different slices from an HH...
Figure 5. A simple layout of the telescope model used in this work. The...
Figure 6. The í µí±¢í µí±£-coverage for the simulated SKA1-Low...
+1 Figure 11. The Largest Cluster Statistic (LCS) is plotted with changing...
Interpreting the HI 21-cm cosmology maps through Largest Cluster Statistics -- I: Impact of the synthetic SKA1-Low observations
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  • Feb 2023
We analyse the evolution of the largest ionized region using the topological and morphological evolution of the redshifted 21-cm signal coming from the neutral hydrogen distribution during the different stages of reionization. For this analysis, we use the "Largest Cluster Statistics" - LCS. We mainly study the impact of the array synthesized beam...
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... mimic this behaviour we subtract the mean from all of the simulated maps considered here. Figure 2 shows that after down-sampling and mean subtraction the reionization history for our maps remains the same. ...
Context 2
... mimic this behaviour we subtract the mean from all of the simulated maps considered here. Figure 2 shows that after down-sampling and mean subtraction the reionization history for our maps remains the same. ...

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