The Impact of Beam Variations on Power Spectrum Estimation for 21 cm Cosmology II: Mitigation of Foreground Systematics for HERA
Honggeun Kim, Nicholas S. Kern, Jacqueline N. Hewitt, Bang D. Nhan,, Joshua S. Dillon, Eloy de Lera Acedo, Scott B. C. Dynes, Nivedita Mahesh,, Nicolas Fagnoni, and David R. DeBoer

TL;DR
This paper investigates how to mitigate calibration-induced foreground contamination in 21 cm cosmology power spectrum measurements with HERA, focusing on gain errors from feed offsets and proposing methods to improve signal recovery.
Contribution
It introduces three mitigation techniques for chromatic gain errors caused by feed nonredundancies, enhancing the accuracy of 21 cm power spectrum estimation.
Findings
Baseline length restriction reduces gain contamination.
Temporal filtering improves calibration stability.
Feed position constraints are necessary for effective mitigation.
Abstract
One key challenge in detecting 21 cm cosmological signal at z > 6 is to separate the cosmological signal from foreground emission. This can be studied in a power spectrum space where the foreground is confined to low delay modes whereas the cosmological signal can spread out to high delay modes. When there is a calibration error, however, chromaticity of gain errors propagates to the power spectrum estimate and contaminates the modes for cosmological detection. The Hydrogen Epoch of Reionization Array (HERA) employs a high-precision calibration scheme using redundancy in measurements. In this study, we focus on the gain errors induced by nonredundancies arising from feed offset relative to the HERA's 14 meter parabolic dish element, and investigate how to mitigate the chromatic gain errors using three different methods: restricting baseline lengths for calibration, smoothing the antenna…
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Taxonomy
TopicsRadio Astronomy Observations and Technology · Superconducting and THz Device Technology · Antenna Design and Optimization
