The Impact of Tandem Redundant/Sky-Based Calibration in MWA Phase II Data Analysis
Zheng Zhang, Jonathan C. Pober, Wenyang Li, Bryna J. Hazelton, Miguel, F. Morales, Cathryn M. Trott, Christopher H. Jordan, Ronniy C. Joseph, Adam, Beardsley, Nichole Barry, Ruby Byrne, Steven J. Tingay, Aman Chokshi, Kenji, Hasegawa, Daniel C. Jacobs, Adam Lanman

TL;DR
This study demonstrates that combining redundant and sky-based calibration methods in MWA Phase II data analysis can significantly improve calibration accuracy, especially in fields with bright radio sources like Fornax A.
Contribution
It provides new evidence that tandem calibration enhances power spectrum results in the presence of bright sources, addressing limitations of sky-based calibration alone.
Findings
Tandem calibration improves power spectrum in EoR1 field.
Bright radio galaxy Fornax A affects calibration performance.
Redundant calibration mitigates model-incompleteness errors.
Abstract
Precise instrumental calibration is of crucial importance to 21-cm cosmology experiments. The Murchison Widefield Array's (MWA) Phase II compact configuration offers us opportunities for both redundant calibration and sky-based calibration algorithms; using the two in tandem is a potential approach to mitigate calibration errors caused by inaccurate sky models. The MWA Epoch of Reionization (EoR) experiment targets three patches of the sky (dubbed EoR0, EoR1, and EoR2) with deep observations. Previous work in \cite{Li_2018} and \cite{Wenyang_2019} studied the effect of tandem calibration on the EoR0 field and found that it yielded no significant improvement in the power spectrum over sky-based calibration alone. In this work, we apply similar techniques to the EoR1 field and find a distinct result: the improvements in the power spectrum from tandem calibration are significant. To…
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