collaborators

15 papers

astro-ph.CO2026

Constraining the neutral hydrogen (HI) distribution

Minal Chhabra, Raghunath Ghara, Somnath Bharadwaj

We constrain the HI distribution by jointly modeling two independent, existing observations of the 21-cm signal, the HI density parameter measured using…

astro-ph.CO2026

Fuzzy Dark Matter Halo Mass Functions at Cosmic Dawn

Raghunath Ghara, Adam Lidz, Daniel Grin +1

In fuzzy dark matter (FDM) cosmological models, wave effects impact astrophysical length scales, suppressing the abundance of small mass dark matter halos, and delaying the earlies…

astro-ph.GA2026

POLAR-II: modeling star formation history of galaxies on the 21-cm signal from Epoch of Reionization

Qing-Bo Ma, Raghunath Ghara, Benedetta Ciardi +6

Galaxies may suffer some starburst and quenched periods in their history due to e.g. galaxy mergers and feedback. However, semi-numerical simulations of the Epoch of Reionization (…

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.CO2025

Asking Fast Radio Bursts for More than Reionization History

Abinash Kumar Shaw, Raghunath Ghara, Paz Beniamini +2

We propose different estimators to probe the intergalactic medium (IGM) during epoch of reionization (EoR) using the dispersion measure () of the fast radio bursts. We co…

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