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First Results from HERA Phase I: Upper Limits on the Epoch of Reionization 21 cm Power Spectrum

Authors :
The HERA Collaboration
Abdurashidova, Zara
Aguirre, James E.
Alexander, Paul
Ali, Zaki S.
Balfour, Yanga
Beardsley, Adam P.
Bernardi, Gianni
Billings, Tashalee S.
Bowman, Judd D.
Bradley, Richard F.
Bull, Philip
Burba, Jacob
Carey, Steve
Carilli, Chris L.
Cheng, Carina
DeBoer, David R.
Dexter, Matt
Acedo, Eloy de Lera
Dibblee-Barkman, Taylor
Dillon, Joshua S.
Ely, John
Ewall-Wice, Aaron
Fagnoni, Nicolas
Fritz, Randall
Furlanetto, Steven R.
Gale-Sides, Kingsley
Glendenning, Brian
Gorthi, Deepthi
Greig, Bradley
Grobbelaar, Jasper
Halday, Ziyaad
Hazelton, Bryna J.
Hewitt, Jacqueline N.
Hickish, Jack
Jacobs, Daniel C.
Julius, Austin
Kern, Nicholas S.
Kerrigan, Joshua
Kittiwisit, Piyanat
Kohn, Saul A.
Kolopanis, Matthew
Lanman, Adam
La Plante, Paul
Lekalake, Telalo
Lewis, David
Liu, Adrian
MacMahon, David
Malan, Lourence
Malgas, Cresshim
Maree, Matthys
Martinot, Zachary E.
Matsetela, Eunice
Mesinger, Andrei
Molewa, Mathakane
Morales, Miguel F.
Mosiane, Tshegofalang
Murray, Steven G.
Neben, Abraham R.
Nikolic, Bojan
Nunhokee, Chuneeta D.
Parsons, Aaron R.
Patra, Nipanjana
Pascua, Robert
Pieterse, Samantha
Pober, Jonathan C.
Razavi-Ghods, Nima
Ringuette, Jon
Robnett, James
Rosie, Kathryn
Sims, Peter
Singh, Saurabh
Smith, Craig
Syce, Angelo
Thyagarajan, Nithyanandan
Williams, Peter K. G.
Zheng, Haoxuan
Publication Year :
2021

Abstract

We report upper-limits on the Epoch of Reionization (EoR) 21 cm power spectrum at redshifts 7.9 and 10.4 with 18 nights of data ($\sim36$ hours of integration) from Phase I of the Hydrogen Epoch of Reionization Array (HERA). The Phase I data show evidence for systematics that can be largely suppressed with systematic models down to a dynamic range of $\sim10^9$ with respect to the peak foreground power. This yields a 95% confidence upper limit on the 21 cm power spectrum of $\Delta^2_{21} \le (30.76)^2\ {\rm mK}^2$ at $k=0.192\ h\ {\rm Mpc}^{-1}$ at $z=7.9$, and also $\Delta^2_{21} \le (95.74)^2\ {\rm mK}^2$ at $k=0.256\ h\ {\rm Mpc}^{-1}$ at $z=10.4$. At $z=7.9$, these limits are the most sensitive to-date by over an order of magnitude. While we find evidence for residual systematics at low line-of-sight Fourier $k_\parallel$ modes, at high $k_\parallel$ modes we find our data to be largely consistent with thermal noise, an indicator that the system could benefit from deeper integrations. The observed systematics could be due to radio frequency interference, cable sub-reflections, or residual instrumental cross-coupling, and warrant further study. This analysis emphasizes algorithms that have minimal inherent signal loss, although we do perform a careful accounting in a companion paper of the small forms of loss or bias associated with the pipeline. Overall, these results are a promising first step in the development of a tuned, instrument-specific analysis pipeline for HERA, particularly as Phase II construction is completed en route to reaching the full sensitivity of the experiment.<br />Comment: Accepted to ApJ. https://reionization.org/science/public-data-release-1/

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.2108.02263
Document Type :
Working Paper
Full Text :
https://doi.org/10.3847/1538-4357/ac1c78