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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 3.

Top (left, right): amplitude and phase spectra on an east–west 29 m baseline for one record at transit of Fornax A. Blue shows the data. Red shows the GLEAM + Fornax A model. Middle: same, but for a 29 m baseline oriented at −30° with respect to north. Bottom: same, but for a 29 m baseline oriented at +30° with respect to north.

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