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Constraining the 21 cm brightness temperature of the IGM at z = 6.6 around LAEs with the murchison widefield array

C. M. Trott*, C. H. Jordan, J. L. B. Line, C. R. Lynch, S. Yoshiura, B. Mckinley, P. Dayal, B. Pindor, A. Hutter, K. Takahashi, R. B. Wayth, N. Barry, A. Beardsley, J. Bowman, R. Byrne, A. Chokshi, B. Greig, K. Hasegawa, B. J. Hazelton, E. HowardD. Jacobs, M. Kolopanis, D. A. Mitchell, M. F. Morales, S. Murray, J. C. Pober, M. Rahimi, S. J. Tingay, R. L. Webster, M. Wilensky, J. S. B. Wyithe, Q. Zheng

*Corresponding author for this work

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