Validation of the HERA Phase I Epoch of Reionization 21 cm Power Spectrum Software Pipeline

Author:

Aguirre James E.ORCID,Murray Steven G.ORCID,Pascua Robert,Martinot Zachary E.,Burba Jacob,Dillon Joshua S.ORCID,Jacobs Daniel C.ORCID,Kern Nicholas S.ORCID,Kittiwisit PiyanatORCID,Kolopanis MatthewORCID,Lanman AdamORCID,Liu AdrianORCID,Whitler Lily,Abdurashidova Zara,Alexander Paul,Ali Zaki S.,Balfour Yanga,Beardsley Adam P.ORCID,Bernardi GianniORCID,Billings Tashalee S.,Bowman Judd D.ORCID,Bradley Richard F.ORCID,Bull PhilipORCID,Carey Steve,Carilli Chris L.ORCID,Cheng Carina,DeBoer David R.ORCID,Dexter Matt,de Lera Acedo Eloy,Ely John,Ewall-Wice AaronORCID,Fagnoni Nicolas,Fritz Randall,Furlanetto Steven R.ORCID,Gale-Sides Kingsley,Glendenning Brian,Gorthi DeepthiORCID,Greig BradleyORCID,Grobbelaar Jasper,Halday Ziyaad,Hazelton Bryna J.ORCID,Hewitt Jacqueline N.ORCID,Hickish Jack,Julius Austin,Kerrigan JoshuaORCID,Kohn Saul A.ORCID,La Plante Paul,Lekalake Telalo,Lewis David,MacMahon David,Malan Lourence,Malgas Cresshim,Maree Matthys,Matsetela Eunice,Mesinger AndreiORCID,Molewa Mathakane,Morales Miguel F.ORCID,Mosiane Tshegofalang,Neben Abraham R.ORCID,Nikolic Bojan,Parsons Aaron R.,Patra NipanjanaORCID,Pieterse Samantha,Pober Jonathan C.ORCID,Razavi-Ghods Nima,Ringuette Jon,Robnett James,Rosie Kathryn,Santos Mario G.ORCID,Sims PeterORCID,Singh SaurabhORCID,Smith Craig,Syce Angelo,Thyagarajan Nithyanandan,Williams Peter K. G.,Zheng Haoxuan

Abstract

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. Our pipeline is able to detect this amplified input signal after suppressing foregrounds with a dynamic range (foreground to noise ratio) of ≳107. 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.

Funder

National Science Foundation

Gordon and Betty Moore Foundation

Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions

INAF PRIN-SKA 2017

Ministero degli Affari Esteri della Cooperazione Internazionale—Direzione Generale per la Promozione del Sistema Paese Progetto di Grande Rilevanza

National Research Foundation of South Africa

Royal Society and the Newton Fund

European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme

NSF AAPF

MIT Pappalardo fellowship

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

STFC Grant

New Frontiers in Research Fund Exploration

Canadian Institute for Advanced Research (CIFAR) Azrieli Global Scholars

Natural Sciences and Engineering Research Council of Canada (NSERC) Discovery Grant and a Discovery Launch Supplement

Sloan Fellowship

William Dawson Scholarship

South African Square Kilometre Array Project and National Research Foundation

NSF CAREER

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 14 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

同舟云学术

1.学者识别学者识别

2.学术分析学术分析

3.人才评估人才评估

"同舟云学术"是以全球学者为主线,采集、加工和组织学术论文而形成的新型学术文献查询和分析系统,可以对全球学者进行文献检索和人才价值评估。用户可以通过关注某些学科领域的顶尖人物而持续追踪该领域的学科进展和研究前沿。经过近期的数据扩容,当前同舟云学术共收录了国内外主流学术期刊6万余种,收集的期刊论文及会议论文总量共计约1.5亿篇,并以每天添加12000余篇中外论文的速度递增。我们也可以为用户提供个性化、定制化的学者数据。欢迎来电咨询!咨询电话:010-8811{复制后删除}0370

www.globalauthorid.com

TOP

Copyright © 2019-2024 北京同舟云网络信息技术有限公司
京公网安备11010802033243号  京ICP备18003416号-3