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From the 1 of 8 linked papers with an AI index.

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20242026
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8 papers

astro-ph.CO2026

Sahyadri: A simulation suite for the cosmology dependence of the Cosmic Web

Saee Dhawalikar, Shadab Alam, Aseem Paranjape +1

The paper presents Sahyadri, a high‑resolution cosmological N‑body simulation suite that varies key cosmological parameters to enable precise studies of the low‑redshift Universe a…

astro-ph.CO2026

Learning Cosmology from Nearest Neighbour Statistics

Atrideb Chatterjee, Arka Banerjee, Francisco Villaescusa-Navarro +1

Extracting cosmological parameters from galaxy/halo catalogues with sub-percent level accuracy is an important aspect of modern cosmology, especially in view of ongoing and upcomin…

astro-ph.CO2026

Nearest Neighbour-Based Statistics for 21cm-Galaxy Cross-Correlations in the Epoch of Reionization

Anirban Chakraborty, Kwanit Gangopadhyay, Arka Banerjee +1

21cm radiation from neutral hydrogen serves as a direct probe of the Epoch of Reionization. However, both its detection and physical interpretation are severely hindered by contami…

astro-ph.CO2025

Geometric Interpretations of the -Nearest Neighbour Distributions

Kwanit Gangopadhyay, Arka Banerjee, Tom Abel

The -Nearest Neighbour Cumulative Distribution Functions are measures of clustering for discrete datasets that are fast and efficient to compute. They are significantly more inf…

astro-ph.CO2025

Boosting HI-Galaxy Cross-Clustering Signal through Higher-Order Cross-Correlations

Eishica Chand, Arka Banerjee, Simon Foreman +1

After reionization, neutral hydrogen (HI) traces the large-scale structure (LSS) of the Universe, enabling HI intensity mapping (IM) to capture the LSS in 3D and constrain key cosm…

astro-ph.CO2025

Exploring Faraday rotation signatures and population bounds for primordial magnetic black holes

Arka Banerjee, Lalit Singh Bhandari, Ashwat Jain +1

Primordial black holes bearing magnetic charges may bypass the constraints imposed by Hawking radiation, thereby enabling reasonable present-day populations, even for masses below…