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20192026
most citedImproving the Epoch of Reionization Power Spectrum Results from Murchison Widefield Array Season 1 Observations

141 citations · 157 across the 10 of their papers we have counts for

collaborators

11 papers

astro-ph.IM2026

Observations of the Cosmic Dawn and Epoch of Reionization with the SKAO: Observational Lessons Learned from Precursors and Pathfinder Instruments

Eloy de Lera Acedo, James Aguirre, Dominic Anstey +34

This chapter summarizes the observational lessons learned after two decades of observations of the Cosmic Dawn (CD) and Epoch of Reionization (EoR) with SKAO pathfinders and precur…

astro-ph.CO2026

The Tracking Tapered Gridded Estimator for the 21-cm power spectrum from the Murchison Widefield Array (MWA) drift scan observations -- III. Improved upper limits at from multiple pointings

Shouvik Sarkar, Khandakar Md Asif Elahi, Samir Choudhuri +5

We analyze zenith-pointing Murchison Widefield Array (MWA) drift scan observations covering with 1…

astro-ph.CO2026

Unbiased Bayesian Inference of Peculiar Motions of Galaxies from Type Ia Supernovae Observations

Ujjwal Upadhyay, Tarun Deep Saini, Shiv K. Sethi

The peculiar motions of galaxies are powerful cosmological probes that trace the growth of structures and the distribution of matter in the universe, providing a means to investiga…

astro-ph.CO2026

The Epoch of Reionization 21 cm Bispectrum at from MWA data II: Smooth Component Filtering

Sukhdeep Singh Gill, Khandakar Md Asif Elahi, Somnath Bharadwaj +2

The 21 cm bispectrum (BS) offers a powerful probe of the Epoch of Reionization (EoR), but its observational access is severely hindered by dominant astrophysical foregrounds. Consi…

astro-ph.CO2025

The EoR 21-cm Bispectrum at from MWA data I: Foregrounds and preliminary upper limits

Sukhdeep Singh Gill, Somnath Bharadwaj, Khandakar Md Asif Elahi +2

We attempt to measure the Epoch of Reionization (EoR) 21-cm bispectrum (BS) using Murchison Widefield Array (MWA) data. We find that $B(k_{1\perp}, k…

astro-ph.GA2025★ 3 cited

A measurement of Galactic synchrotron emission using MWA drift scan observations

Suman Chatterjee, Shouvik Sarkar, Samir Choudhuri +4

Studying the diffuse Galactic synchrotron emission (hereafter, DGSE) at arc-minute angular scale is important to remove the foregrounds for the cosmological 21-cm observations. Sta…

astro-ph.CO2025

Scalar-induced gravitational waves from coherent initial states

Dipayan Mukherjee, H. V. Ragavendra, Shiv K. Sethi

We investigate the impact of statistical inhomogeneity and anisotropy in primordial scalar perturbations on the scalar-induced gravitational waves (SIGW). Assuming inflationary qua…

astro-ph.CO2025★ 2 cited

21 cm Signal from the Thermal Evolution of Lyman- during Cosmic Dawn

Janakee Raste, Shiv K. Sethi

The Lyman- photons couple the spin temperature of neutral hydrogen (HI) to the kinetic temperature during the era of cosmic dawn. During this process, they also exchange energy…

astro-ph.CO2024

The Tracking Tapered Gridded Estimator for the 21-cm power spectrum from MWA drift scan observations II: The Missing Frequency Channels

Khandakar Md Asif Elahi, Somnath Bharadwaj, Suman Chatterjee +4

Missing frequency channels pose a problem for estimating the redshifted 21-cm power spectrum (PS) from radio-interferometric visibility data. This is parti…

astro-ph.CO2024★ 11 cited

The Tracking Tapered Gridded Estimator for the 21-cm power spectrum from MWA drift scan observations I: Validation and preliminary results

Suman Chatterjee, Khandakar Md Asif Elahi, Somnath Bharadwaj +4

Drift scan observations provide the broad sky coverage and instrumental stability needed to measure the Epoch of Reionization (EoR) 21-cm signal. In such observations, the telescop…

astro-ph.IM2019★ 141 cited

Improving the Epoch of Reionization Power Spectrum Results from Murchison Widefield Array Season 1 Observations

N. Barry, M. Wilensky, C. M. Trott +27

Measurements of 21 cm Epoch of Reionization (EoR) structure are subject to systematics originating from both the analysis and the observation conditions. Using 2013 data from the M…