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How a radio telescope doubled its power to glimpse the universe's first galaxies

S. J. Tingay, M. Johnston-Hollitt, R. B. Wayth, T. A. Booler, J. Jones, Y. Wu, J. Gan, G. Sleap, A. McPhail, C. Wintle, A. Williams, C. J. Phillips, L. Verduyn, D. Emrich, P. Giersch, C. J. Riseley, S. Duchesne, C. M. Trott, D. Null, B. W. Myers, C. D. Nunhokee, N. Barry, L. Dressler, J. Ducharme, B. Hazelton, M. Lee, E. Lilleskov, M. Morales, J. Pober, Zhiqiang Shen, Xiang-ping Wu, Xiaoyu Hong, M. D. Filipović, S. E. Tremblay, M. Walker

June 1, 2026

The Murchison Widefield Array in Australia completed a major upgrade: new digital receivers and a faster correlator now let it use all 256 antenna tiles simultaneously, whereas before it could only process 128 at a time. This doubles sensitivity and quadruples the number of independent measurements, dramatically improving its ability to detect faint radio signals from the universe's first galaxies during reionization.
Published as The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised arXiv:2606.01644
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