activity
20172026
most citedThe Present and Future of QCD

67 citations · 925 across the 111 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

5 papers · 1 filter

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.CO2019

Simulated Predictions for HI at with the Ooty Wide Field Array (OWFA) -- II: Foreground Avoidance

Suman Chatterjee, Somnath Bharadwaj, Visweshwar Ram Marthi

Considering the upcoming OWFA, we use simulations of the foregrounds and the HI 21-cm intensity mapping signal to identify the modes where th…

astro-ph.CO2018

A Spherical Harmonic Analysis of the Ooty Wide Field Array (OWFA) Visibility Signal

Suman Chatterjee, Somnath Bharadwaj

Considering redshifted -cm intensity mapping with the upcoming OWFA whose field of view subtends in the N-S direction, we present a formalism which relates th…

astro-ph.CO2018

On the Prospects of Measuring the Cosmic Dawn 21-cm Power Spectrum using the Upgraded Giant Meterwave Radio Telescope (uGMRT)

Suman Chatterjee, Somnath Bharadwaj

A recent observation by the EDGES collaboration shows a strong absorption signal in the global 21-cm spectrum from around a redshift of . This absorption is stronger than t…

astro-ph.CO2017★ 7 cited

Simulating the z = 3.35 HI 21-cm visibility signal for the Ooty Wide Field Array(OWFA)

Suman Chatterjee, S. Bharadwaj, V. R. Marthi

The upcoming Ooty Wide Field Array (OWFA) will operate at which corresponds to the redshifted 21-cm signal from neutral hydrogen (HI) at z = 3.35. We present t…