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papers

Publications (25)

astro-ph.IM2016

The Murchison Widefield Array 21 cm Power Spectrum Analysis Methodology

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

astro-ph.IM2016

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

astro-ph.GA2014

First Look Murchison Widefield Array observations of Abell 3667

L. Hindson, M. Johnston-Hollitt, N. Hurley-Walker +51

astro-ph.GA2014

The first Murchison Widefield Array low frequency radio observations of cluster scale non-thermal emission: the case of Abell 3667

L. Hindson, M. Johnston-Hollitt, N. Hurley-Walker +51

astro-ph.IM2015

The low-frequency environment of the Murchison Widefield Array: radio-frequency interference analysis and mitigation

A. R. Offringa, R. B. Wayth, N. Hurley-Walker +62

astro-ph.IM2015

Foregrounds in Wide-Field Redshifted 21 cm Power Spectra

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

astro-ph.IM2015

Ionospheric modelling using GPS to calibrate the MWA. 1: Comparison of first order ionospheric effects between GPS models and MWA observations

B. S. Arora, J. Morgan, S. M. Ord +56

astro-ph.IM2018

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

astro-ph.IM2017

A high resolution foreground model for the MWA EoR1 field: model and implications for EoR power spectrum analysis

P. Procopio, R. B. Wayth, J. Line +23

astro-ph.IM2016

First Season MWA EoR Power Spectrum Results at Redshift 7

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

astro-ph.HE2014

Modelling of the Spectral Energy Distribution of Fornax A: Leptonic and Hadronic Production of High Energy Emission from the Radio Lobes

B. McKinley, R. Yang, M. López-Caniego +52

astro-ph.IM2014

WSClean: an implementation of a fast, generic wide-field imager for radio astronomy

A. R. Offringa, B. McKinley, N. Hurley-Walker +50

astro-ph.CO2015

Confirmation of Wide-Field Signatures in Redshifted 21 cm Power Spectra

Nithyanandan Thyagarajan, Daniel C. Jacobs, Judd D. Bowman +52

astro-ph.GA2015

Broadband Spectral Modeling of the Extreme Gigahertz-Peaked Spectrum Radio Source PKS B0008-421

J. R. Callingham, B. M. Gaensler, R. D. Ekers +40

astro-ph.GA2017

Spectral energy distribution and radio halo of NGC 253 at low radio frequencies

A. D. Kapinska, L. Staveley-Smith, R. Crocker +67

astro-ph.HE2016

High-energy sources at low radio frequency: the Murchison Widefield Array view of Fermi blazars

M. Giroletti, F. Massaro, R. D'Abrusco +54

astro-ph.CO2015

Empirical Covariance Modeling for 21 cm Power Spectrum Estimation: A Method Demonstration and New Limits from Early Murchison Widefield Array 128-Tile Data

Joshua S. Dillon, Abraham R. Neben, Jacqueline N. Hewitt +52

astro-ph.IM2016

Parametrising Epoch of Reionization foregrounds: A deep survey of low-frequency point-source spectra with the MWA

A. R. Offringa, C. M. Trott, N. Hurley-Walker +38

astro-ph.CO2016

Delay Spectrum with Phase-Tracking Arrays: Extracting the HI power spectrum from the Epoch of Reionization

Sourabh Paul, Shiv K. Sethi, Miguel F. Morales +51

astro-ph.GA2016

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

astro-ph.CO2016

First Limits on the 21 cm Power Spectrum during the Epoch of X-ray heating

A. Ewall-Wice, Joshua S. Dillon, J. N. Hewitt +62

astro-ph.IM2016

CHIPS: The Cosmological HI Power Spectrum Estimator

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

astro-ph.IM2016

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

astro-ph.IM2015

The Murchison Widefield Array Correlator

S. M. Ord, B. Crosse, D. Emrich +64

astro-ph.IM2013

On the detection and tracking of space debris using the Murchison Widefield Array. I. Simulations and test observations demonstrate feasibility

S. J. Tingay, D. L. Kaplan, B. McKinley +60