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Improved Constraints on the 21 cm EoR Power Spectrum and the X-Ray Heating of the IGM with HERA Phase I Observations

T. Collaboration, Z. Abdurashidova, T. Adams, J. Aguirre, P. Alexander, Z. Ali, R. Baartman, Y. Balfour, R. Barkana, A. Beardsley, G. Bernardi, T. Billings, J. Bowman, R. Bradley, D. Breitman, P. Bull, J. Burba, S. Carey, C. Carilli, C. Cheng, S. Choudhuri, D. DeBoer, E. Acedo, M. Dexter, J. Dillon, J. Ely, A. Ewall-Wice, N. Fagnoni, A. Fialkov, R. Fritz, S. Furlanetto, K. Gale-Sides, H. Garsden, B. Glendenning, A. Gorce, D. Gorthi, B. Greig, J. Grobbelaar, Z. Halday, B. Hazelton, S. Heimersheim, J. Hewitt, J. Hickish, D. Jacobs, A. Julius, N. Kern, J. Kerrigan, P. Kittiwisit, S. Kohn, M. Kolopanis, A. Lanman, P. La Plante, D. Lewis, A. Liu, A. Loots, Y. Ma, D. MacMahon, L. Malan, K. Malgas, C. Malgas, M. Maree, B. Marero, Z. Martinot, L. McBride, A. Mesinger, J. Mirocha, M. Molewa, M. Morales, T. Mosiane, J. Muñoz, S. Murray, V. Nagpal, A. Neben, B. Nikolic, C. Nunhokee, H. Nuwegeld, A. Parsons, R. Pascua, N. Patra, S. Pieterse, Y. Qin, N. Razavi-Ghods, J. Robnett, K. Rosie, M. Santos, P. Sims, S. Singh, C. Smith, H. Swarts, N. Thyagarajan, M. Wilensky, P. Williams, P. van Wyngaarden, and H. Zheng. (2022)cite arxiv:2210.04912Comment: 55 pages, 37 figures. Submitted to ApJ. Corresponding author: Joshua S. Dillon.

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Characterization Of Inpaint Residuals In Interferometric Measurements of the Epoch Of ReionizationM. Pagano, J. Liu, A. Liu, N. Kern, A. Ewall-Wice, P. Bull, R. Pascua, S. Ravanbakhsh, Z. Abdurashidova, T. Adams and 68 other author(s). (2022)cite arxiv:2210.14927Comment: 26 pages, 18 figures.Detection of Cosmic Structures using the Bispectrum Phase. II. First Results from Application to Cosmic Reionization Using the Hydrogen Epoch of Reionization ArrayN. Thyagarajan, C. Carilli, B. Nikolic, J. Kent, A. Mesinger, N. Kern, G. Bernardi, S. Matika, Z. Abdurashidova, J. Aguirre and 62 other author(s). (2020)cite arxiv:2005.10275Comment: 22 pages, 12 figures (including sub-figures). Accepted for publication in PhRvD. Abstract may be slightly abridged compared to the actual manuscript due to length limitations on arXiv.Methods of Error Estimation for Delay Power Spectra in $21\,cm$ CosmologyJ. Tan, A. Liu, N. Kern, Z. Abdurashidova, J. Aguirre, P. Alexander, Z. Ali, Y. Balfour, A. Beardsley, G. Bernardi and 64 other author(s). (2021)cite arxiv:2103.09941Comment: 34 Pages, 9 Figures, 4 Tables.Measuring HERA's primary beam in-situ: methodology and first resultsC. Nunhokee, A. Parsons, N. Kern, B. Nikolic, J. Pober, G. Bernardi, C. Carilli, Z. Abdurashidova, J. Aguirre, P. Alexander und 57 andere Autor(en). (2020)cite arxiv:2005.12174Comment: 22 pages, 22 figures, accepted for publication in ApJ.Improved Constraints on the 21 cm EoR Power Spectrum and the X-Ray Heating of the IGM with HERA Phase I ObservationsT. Collaboration, Z. Abdurashidova, T. Adams, J. Aguirre, P. Alexander, Z. Ali, R. Baartman, Y. Balfour, R. Barkana, A. Beardsley und 84 andere Autor(en). (2022)cite arxiv:2210.04912Comment: 55 pages, 37 figures. Submitted to ApJ. Corresponding author: Joshua S. Dillon.Direct Optimal Mapping for 21cm Cosmology: A Demonstration with the Hydrogen Epoch of Reionization ArrayZ. Xu, J. Hewitt, K. Chen, H. Kim, J. Dillon, N. Kern, M. Morales, B. Hazelton, R. Byrne, N. Fagnoni und 71 andere Autor(en). (2022)cite arxiv:2204.06021Comment: 16 pages, 10 figures, 2 tables, submitted to ApJ.HERA Phase I Limits on the Cosmic 21-cm Signal: Constraints on Astrophysics and Cosmology During the Epoch of ReionizationT. Collaboration, Z. Abdurashidova, J. Aguirre, P. Alexander, Z. Ali, Y. Balfour, R. Barkana, A. Beardsley, G. Bernardi, T. Billings und 74 andere Autor(en). (2021)cite arxiv:2108.07282Comment: 40 pages, 19 figures, submitted to ApJ.A Real Time Processing system for big data in astronomy: Applications to HERA.P. Plante, P. Williams, M. Kolopanis, J. Dillon, A. Beardsley, N. Kern, M. Wilensky, Z. Ali, Z. Abdurashidova, J. Aguirre und 65 andere Autor(en). Astron. Comput., (2021)

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Improved Constraints on the 21 cm EoR Power Spectrum and the X-Ray Heating of the IGM with HERA Phase I Observations

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Improved Constraints on the 21 cm EoR Power Spectrum and the X-Ray Heating of the IGM with HERA Phase I Observations