Validation of the hera phase i epoch of reionization 21 cm power spectrum software pipeline
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Date
2022
Journal Title
Journal ISSN
Volume Title
Publisher
IOP Publishing
Abstract
We describe the validation of the HERA Phase I software pipeline by a series of modular tests, building up to an
end-to-end simulation. The philosophy of this approach is to validate the software and algorithms used in the Phase
I upper-limit analysis on wholly synthetic data satisfying the assumptions of that analysis, not addressing whether
the actual data meet these assumptions. We discuss the organization of this validation approach, the specific
modular tests performed, and the construction of the end-to-end simulations. We explicitly discuss the limitations
in scope of the current simulation effort. With mock visibility data generated from a known analytic power
spectrum and a wide range of realistic instrumental effects and foregrounds, we demonstrate that the current
pipeline produces power spectrum estimates that are consistent with known analytic inputs to within thermal noise
levels (at the 2σ level) for k > 0.2h Mpc−1 for both bands and fields considered. Our input spectrum is intentionally
amplified to enable a strong “detection” at k ∼ 0.2 h Mpc−1
—at the level of ∼25σ—with foregrounds dominating
on larger scales and thermal noise dominating at smaller scales.
Description
Keywords
Reionization, Astronomical simulations, Astronomy data analysis, Power spectrum, HERA phase I
Citation
Aguirre, J. E. et al. (2022). Validation of the hera phase i epoch of reionization 21 cm power spectrum software pipeline. Astrophysical Journal, 924 (2). https://doi.org/10.3847/1538-4357/ac32cd