activity
20242026
collaborators

6 papers

astro-ph.CO2026

Overview of 21cm Experiments at high redshift with SKAO

CD Science Working Group, Gianni Bernardi, Daniela Breitman +81

We provide an overview of the eight SKAO Science Book chapters that motivate the Epoch of Reionisation and Cosmic Dawn experiments with SKA-Low. We describe the individual SKA-Low…

astro-ph.CO2026

Imaging the 21-cm Signal from the Cosmic Dawn & Epoch of Reionization and the Connection with the Global Signal

Satadru Bag, Michele Bianco, Samir Choudhuri +12

The original baseline design for SKA-Low was motivated by the ability to produce tomographic images of the redshifted 21-cm signal, thus allowing the research field to move beyond…

astro-ph.CO2026

Enhancing the detectability of ionized Regions during the Epoch of Reionization

Rutvik Ashish Mahajan, Raghunath Ghara, Nishant Pradeep Deo +1

We present an improved matched filter method for detecting large ionized regions in 21 cm observations of the Epoch of Reionization. In addition to detection, the method constrains…

astro-ph.CO2026

Probing ionized bubbles around luminous sources during reionization with SKA 21-cm observations

Arnab Mishra, Kanan Kumar Datta, Chandra Shekhar Murmu +3

Detecting and characterizing individual ionized bubbles during the Epoch of Reionization (EoR) using the redshifted HI 21-cm signal provides a direct probe of the early ionizing so…

astro-ph.CO2025

The Effect of Large Optical Depths on the Non-Gaussian 21-cm signal from Cosmic Dawn

Iffat Nasreen, Kanan K. Datta, Abinash K. Shaw +6

During the Cosmic Dawn (CD), the HI 21-cm optical depth ( ) in the intergalactic medium can become significantly large. Consequently, the second and higher-order terms of

astro-ph.CO2024

Detecting ionized bubbles around luminous sources during the reionization era using HI 21-cm signal

Arnab Mishra, Chandra Shekhar Murmu, Kanan K. Datta +4

Measuring the properties of the intergalactic medium (IGM) and sources during the Epoch of Reionization (EoR) is of immense importance. We explore the prospects of probing the IGM…