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Imaging and Modeling Data from the Hydrogen Epoch of Reionization Array

  • Authors: C. L. Carilli, N. Thyagarajan, J. Kent, B. Nikolic, K. Gale-Sides, N. S. Kern, G. Bernardi, A. Mesinger, S. Matika, Zara Abdurashidova, James E. Aguirre, Paul Alexander, Zaki S. Ali, Yanga Balfour, Adam P. Beardsley, Tashalee S. Billings, Judd D. Bowman, Richard F. Bradley, Phil Bull, Jacob Burba, Carina Cheng, David R. DeBoer, Matt Dexter, Eloy de Lera Acedo, Joshua S. Dillon, Aaron Ewall-Wice, Nicolas Fagnoni, Randall Fritz, Steve R. Furlanetto, Kingsley Gale-Sides, Brian Glendenning, Deepthi Gorthi, Bradley Greig, Jasper Grobbelaar, Ziyaad Halday, Bryna J. Hazelton, Jacqueline N. Hewitt, Jack Hickish, Daniel C. Jacobs, Alec Josaitis, Austin Julius, Joshua Kerrigan, Honggeun Kim, Piyanat Kittiwisit, Saul A. Kohn, Matthew Kolopanis, Adam Lanman, Paul La Plante, Telalo Lekalake, Adrian Liu, David MacMahon, Lourence Malan, Cresshim Malgas, Matthys Maree, Zachary E. Martinot, Eunice Matsetela, Mathakane Molewa, Miguel F. Morales, Tshegofalang Mosiane, Abraham R. Neben, Juan Mena Parra, Aaron R. Parsons, Nipanjana Patra, Samantha Pieterse, Jonathan C. Pober, Nima Razavi-Ghods, James Robnett, Kathryn Rosie, Peter Sims, Angelo Syce, Peter K. G. Williams, and Haoxuan Zheng

2020 The Astrophysical Journal Supplement Series 247 67.

  • Provider: AAS Journals

Caption: Figure 10.

Left: red is the visibility amplitude spectrum for the GLEAM plus the scaled-down diffuse sky model (as show in Figure 8) for a 29 m baseline. Blue is the same, but for a 44 m baseline. Right: red shows the visibility amplitude spectrum for the GLEAM plus the scaled diffuse sky model (as show in Figure 8) for an east–west 29 m baseline. Black shows a 29 m baseline oriented 30° counterclockwise from north. Blue shows a 29 m baseline at 30° clockwise from north.

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