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  • The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised
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The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised

Fuente: arXiv
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Bibliographic Details
Main Authors: Tingay, S. J., Johnston-Hollitt, M., Wayth, R. B., Booler, T. A., Jones, J., Wu, Y., Gan, J., Sleap, G., McPhail, A., Wintle, C., Williams, A., Phillips, C. J., Verduyn, L., Emrich, D., Giersch, P., Riseley, C. J., Duchesne, S., Trott, C. M., Null, D., Myers, B. W., Nunhokee, C. D., Barry, N., Dressler, L., Ducharme, J., Hazelton, B., Lee, M., Lilleskov, E., Morales, M., Pober, J., Shen, Zhiqiang, Wu, Xiang-ping, Hong, Xiaoyu, Filipović, M. D., Tremblay, S. E., Walker, M.
Format: Preprint
Published: 2026
Subjects:
Instrumentation and Methods for Astrophysics
Cosmology and Nongalactic Astrophysics
Online Access:
Acceder al recurso
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Internet

https://arxiv.org/abs/2606.01644

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