Validation of the HERA Phase i Epoch of Reionization 21 cm Power Spectrum Software Pipeline
Authors
Pascua, R
Martinot, ZE
Burba, J
Whitler, L
Abdurashidova, Z
Alexander, P
Ali, ZS
Balfour, Y
Billings, TS
Carey, S
Cheng, C
Dexter, M
De Lera Acedo, E
Ely, J
Fagnoni, N
Fritz, R
Gale-Sides, K
Glendenning, B
Grobbelaar, J
Halday, Z
Hickish, J
Julius, A
La Plante, P
Lekalake, T
Lewis, D
Macmahon, D
Malan, L
Malgas, C
Maree, M
Matsetela, E
Molewa, M
Mosiane, T
Nikolic, B
Parsons, AR
Pieterse, S
Razavi-Ghods, N
Ringuette, J
Robnett, J
Rosie, K
Smith, C
Syce, A
Thyagarajan, N
Williams, PKG
Zheng, H
Publication Date
2022Journal Title
Astrophysical Journal
ISSN
0004-637X
Publisher
American Astronomical Society
Volume
924
Issue
2
Language
en
Type
Article
This Version
VoR
Metadata
Show full item recordCitation
Aguirre, J., Murray, S., Pascua, R., Martinot, Z., Burba, J., Dillon, J., Jacobs, D., 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
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 2 sigma
level) for k > 0.2 h/Mpc for both bands and fields considered. Our input
spectrum is intentionally amplified to enable a strong `detection' at k ~0.2
h/Mpc -- at the level of ~25 sigma -- with foregrounds dominating on larger
scales, and thermal noise dominating at smaller scales. Our pipeline is able to
detect this amplified input signal after suppressing foregrounds with a dynamic
range (foreground to noise ratio) of > 10^7. Our validation test suite
uncovered several sources of scale-independent signal loss throughout the
pipeline, whose amplitude is well-characterized and accounted for in the final
estimates. We conclude with a discussion of the steps required for the next
round of data analysis.
Keywords
310, Galaxies and Cosmology
Sponsorship
National Science Foundation (NSF) (1636646)
National Science Foundation (NSF) (1836019)
Gordon and Betty Moore Foundation (GBMF) (N/A)
Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) (CE170100013)
INAF PRIN-SKA 2017 (1.05.01.88.04)
Ministero degli Affari Esteri della Cooperazione Internazionale—Direzione Generale per la Promozione del Sistema Paese Progetto di Grande Rilevanza (ZA18GR02)
National Research Foundation of South Africa (113121)
Royal Society and the Newton Fund (NA150184)
National Research Foundation of South Africa (103424)
European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (948764)
NSF AAPF (1701536)
MIT Pappalardo fellowship (N/A)
New Frontiers in Research Fund Exploration grant program, the Canadian Institute for Advanced Research (CIFAR) Azrieli Global Scholars program, a Natural Sciences and Engineering Research Council of C (N/A)
STFC Grant (ST/T000341/1)
New Frontiers in Research Fund Exploration (N/A)
Canadian Institute for Advanced Research (CIFAR) Azrieli Global Scholars (N/A)
Natural Sciences and Engineering Research Council of Canada (NSERC) Discovery Grant and a Discovery Launch Supplement (N/A)
Sloan Fellowship (N/A)
William Dawson Scholarship (N/A)
South African Square Kilometre Array Project and National Research Foundation (84156)
NSF CAREER (1455151)
Identifiers
apjac32cd, ac32cd, aas31639
External DOI: https://doi.org/10.3847/1538-4357/ac32cd
This record's URL: https://www.repository.cam.ac.uk/handle/1810/333060
Rights
Licence:
http://creativecommons.org/licenses/by/4.0/
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