Aguirre, James E.Murray, Steven G.Santos, Mario G.2022-02-072022-02-072022Aguirre, 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/ac32cd1538-4357https://doi.org/10.3847/1538-4357/ac32cdhttp://hdl.handle.net/10566/7164We 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.enReionizationAstronomical simulationsAstronomy data analysisPower spectrumHERA phase IArticle