Beam Perturbation impact on Calibration and the 21cm Power Spectrum

We study the impact of broken dipoles in the Murchison Widefield Array (MWA) on the detectibility of a signal from the Epoch of Reionisation.

The results are published in: Ronniy C Joseph, C M Trott, R B Wayth, A Nasirudin, Calibration and 21-cm power spectrum estimation in the presence of antenna beam variations, Monthly Notices of the Royal Astronomical Society, Volume 492, Issue 2, February 2020, Pages 2017–2028, https://doi.org/10.1093/mnras/stz3375

Name		Name	Last commit message	Last commit date
Latest commit History 212 Commits
Data		Data
Notebooks		Notebooks
Testing		Testing
approximations		approximations
numerical_simulations		numerical_simulations
LICENSE.md		LICENSE.md
Plot_Calibrated_Error_Comparison.py		Plot_Calibrated_Error_Comparison.py
Plot_Calibrated_Errors_MWA.py		Plot_Calibrated_Errors_MWA.py
Plot_Calibrated_Uncalibrated_Comparison.py		Plot_Calibrated_Uncalibrated_Comparison.py
Plot_Fiducial_PS.py		Plot_Fiducial_PS.py
Plot_Gain_Error_PS.py		Plot_Gain_Error_PS.py
Plot_MWA_uv_distribution.py		Plot_MWA_uv_distribution.py
Plot_Sky_Beam_Total_Covariances.py		Plot_Sky_Beam_Total_Covariances.py
README.md		README.md
__init__.py		__init__.py
analytic_covariance.py		analytic_covariance.py
generaltools.py		generaltools.py
plottools.py		plottools.py
powerspectrum.py		powerspectrum.py
radiotelescope.py		radiotelescope.py
skymodel.py		skymodel.py

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Beam Perturbation impact on Calibration and the 21cm Power Spectrum

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