Analysis of realistic HI 21-cm maps from Epoch of Reionization using Largest Cluster Statistics (LCS)

S. Dasgupta, S. Bag, S. Majumdar, S. Dutta
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Abstract

Using the topological and morphological evolution of neutral hydrogen distribution during the different stages of the Epoch of Reionization (EoR), we try to reveal the nature of the ionizing sources and the astrophysical processes in the Intergalactic Medium (IGM) during this period by studying the evolution of the largest ionized region (via the Largest Cluster Statistics - LCS). We show that It can identify the difference between two distinct reionization scenarios - inside-out and outside-in, even when realistic observational conditions are taken into account i.e. the simulated HI 21cm maps are initially translated to a lower resolution, then corrupted with a simulated Gaussian noise having an RMS value of $\sim 3mK$ in line with the future SKA1-low observations. Afterwards, the effect of the beam was simulated and incorporated into the maps, and then the images are analyzed via LCS. Additionally, we use Shapefinders (SFs) to investigate the morphology of ionized volumes as they change in different reionization models. We observed that the greatest ionized volume abruptly expands solely in terms of its third SF after percolation while the first two SFs stay almost constant. Ergo, when approaching percolation, the ionized hydrogen in these circumstances becomes very filamentary, with a characteristic cross-section’ that differs between source models.
利用最大聚类统计(LCS)分析再电离时代真实HI 21厘米地图
利用再电离时代(EoR)不同阶段中性氢分布的拓扑和形态演变,通过研究最大电离区域(通过最大星团统计- LCS)的演变,试图揭示这一时期星系际介质(IGM)中电离源的性质和天体物理过程。我们表明,即使考虑到现实的观测条件,它也可以识别两种不同的再电离情景之间的差异,即模拟的HI 21cm图最初被转换为较低的分辨率,然后被模拟的高斯噪声破坏,其RMS值为$\sim 3mK$,与未来的ska1低观测值一致。然后,模拟光束的影响并将其纳入地图中,然后通过LCS对图像进行分析。此外,我们使用shapefinder (sf)来研究电离体积在不同再电离模型中变化的形态。我们观察到,最大的电离体积在渗透后仅以其第三个SF突然膨胀,而前两个SF几乎保持不变。因此,当接近渗透时,在这些情况下电离的氢变得非常丝状,具有不同源模型的特征截面。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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