activity
19982021
most citedWSClean: an implementation of a fast, generic wide-field imager for radio astronomy

937 citations · 6.8k across the 82 of their papers we have counts for

collaborators

84 papers

astro-ph.CO2021★ 9 cited

On the detection of a cosmic dawn signal in the radio background

Saurabh Singh, Jishnu Nambissan T., Ravi Subrahmanyan +6

The astrophysics of cosmic dawn, when star formation commenced in the first collapsed objects, is predicted to be revealed as spectral and spatial signatures in the cosmic radio ba…

astro-ph.IM2021★ 14 cited

A Floating Octave Bandwidth Cone-Disc Antenna for Detection of Cosmic Dawn

Agaram Raghunathan, Ravi Subrahmanyan, N. Udaya Shankar +9

The critical component of radio astronomy radiometers built to detect redshifted 21-cm signals from Cosmic Dawn is the antenna element. We describe the design and performance of an…

astro-ph.IM2021★ 55 cited

SARAS 3 CD/EoR Radiometer: Design and Performance of the Receiver

Jishnu Nambissan T., Ravi Subrahmanyan, R. Somashekar +6

SARAS is an ongoing experiment aiming to detect the redshifted global 21-cm signal expected from Cosmic Dawn (CD) and the Epoch of Reionization (EoR). Standard cosmological models…

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…

astro-ph.GA2018★ 12 cited

The Murchison Widefield Array Transients Survey (MWATS). A search for low frequency variability in a bright Southern hemisphere sample

M. E. Bell, Tara Murphy, P. J. Hancock +38

We report on a search for low-frequency radio variability in 944 bright (> 4Jy at 154 MHz) unresolved, extragalactic radio sources monitored monthly for several years with the Murc…

astro-ph.IM2018★ 57 cited

Comparing Redundant and Sky Model Based Interferometric Calibration: A First Look with Phase II of the MWA

W. Li, J. C. Pober, B. J. Hazelton +53

Interferometric arrays seeking to measure the 21 cm signal from the Epoch of Reionization must contend with overwhelmingly bright emission from foreground sources. Accurate recover…