activity
20142023
most citedFirst Season MWA EoR Power Spectrum Results at Redshift 7

170 citations · 1k across the 18 of their papers we have counts for

collaborators
Showing astro-ph.IMShow all

9 papers · 1 filter

astro-ph.IM2022

Characterization of the John A. Galt telescope for radio holography with CHIME

Alex Reda, Tristan Pinsonneault-Marotte, Meiling Deng +21

The Canadian Hydrogen Intensity Mapping Experiment (CHIME) will measure the 21 cm emission of astrophysical neutral hydrogen to probe large scale structure at redshifts z=0.8-2.5.…

astro-ph.IM2021★ 3 cited

The Hydrogen Intensity and Real-time Analysis eXperiment: 256-Element Array Status and Overview

Devin Crichton, Moumita Aich, Adam Amara +97

The Hydrogen Intensity and Real-time Analysis eXperiment (HIRAX) is a radio interferometer array currently in development, with an initial 256-element array to be deployed at the S…

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…

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.IM2016★ 72 cited

The Murchison Widefield Array 21 cm Power Spectrum Analysis Methodology

Daniel C. Jacobs, B. J. Hazelton, C. M. Trott +61

We present the 21 cm power spectrum analysis approach of the Murchison Widefield Array Epoch of Reionization project. In this paper, we compare the outputs of multiple pipelines fo…

astro-ph.IM2016★ 93 cited

The Importance of Wide-field Foreground Removal for 21 cm Cosmology: A Demonstration With Early MWA Epoch of Reionization Observations

J. C. Pober, B. J. Hazelton, A. P. Beardsley +66

In this paper we present observations, simulations, and analysis demonstrating the direct connection between the location of foreground emission on the sky and its location in cosm…

astro-ph.IM2016★ 123 cited

CHIPS: The Cosmological HI Power Spectrum Estimator

Cathryn M. Trott, Bart Pindor, Pietro Procopio +49

Detection of the cosmological neutral hydrogen signal from the Epoch of Reionization, and estimation of its basic physical parameters, is the principal scientific aim of many curre…

astro-ph.IM2015★ 161 cited

Foregrounds in Wide-Field Redshifted 21 cm Power Spectra

Nithyanandan Thyagarajan, Daniel C. Jacobs, Judd D. Bowman +61

Detection of 21~cm emission of HI from the epoch of reionization, at redshifts z>6, is limited primarily by foreground emission. We investigate the signatures of wide-field measure…

astro-ph.IM2014★ 10 cited

Study of Redshifted HI from the Epoch of Reionization with Drift scan

Sourabh Paul, Shiv K. Sethi, Ravi Subrahmanyan +37

The detection of the Epoch of Reionization (EoR) in the redshifted 21-cm line is a challenging task. Here we formulate the detection of the EoR signal using the drift scan strategy…