activity
20092022
most citedThe Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies

1.3k citations · 4.1k across the 41 of their papers we have counts for

collaborators

41 papers

astro-ph.EP2022

Probing the Plasma Tail of Interstellar Comet 2I/Borisov

P K Manoharan, Phil Perillat, C J Salter +8

We present an occultation study of compact radio sources by the plasma tail of interstellar Comet 2I/Borisov (C/2019 Q4) both pre- and near-perihelion using the Arecibo and Green B…

astro-ph.GA2021

Arecibo-Green Bank-LOFAR Carbon Radio Recombination Line observations toward cold HI Clouds

D. Anish Roshi, W. M. Peters, K. L. Emig +4

We present results from a search for radio recombination lines in three HI self-absorbing (HISA) clouds at 750 MHz and 321 MHz with the Robert C. Byrd Green Bank Telescope (GBT), a…

astro-ph.GA2021

Long-term meter wavelength variability study of Blazar J1415+1320 using the Ooty Radio Telescope

Sravani Vaddi, P. K. Manoharan, Anish Roshi

J1415+1320 is a well-studied blazar that exhibits strong flux density variability at a wide range of radio frequencies (2.4 230~GHz). In this letter, we present a variability s…

astro-ph.IM2016★ 170 cited

First Season MWA EoR Power Spectrum Results at Redshift 7

A. P. Beardsley, B. J. Hazelton, I. S. Sullivan +63

The Murchison Widefield Array (MWA) has collected hundreds of hours of Epoch of Reionization (EoR) data and now faces the challenge of overcoming foreground and systematic contamin…

astro-ph.GA2016★ 80 cited

Low frequency observations of linearly polarized structures in the interstellar medium near the south Galactic pole

Emil Lenc, B. M. Gaensler, X. H. Sun +76

We present deep polarimetric observations at 154 MHz with the Murchison Widefield Array (MWA), covering 625 deg^2 centered on RA=0 h, Dec=-27 deg. The sensitivity available in our…

astro-ph.IM2016★ 34 cited

A High Reliability Survey of Discrete Epoch of Reionization Foreground Sources in the MWA EoR0 Field

P. A. Carroll, J. Line, M. F. Morales +61

Detection of the Epoch of Reionization HI signal requires a precise understanding of the intervening galaxies and AGN, both for instrumental calibration and foreground removal. We…