Verifying the Australian MWA EoR pipeline I: 21-cm sky model and correlated measurement density von Line, J.L.B., Trott, C.M., Cook, J.H., Greig, B., Barry, N., Jordan, C.H.

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Constraining the 21 cm brightness temperature of the IGM at z = 6.6 around LAEs with the murchison widefield array von Trott, Cathryn, Jordan, Chris, Line, J.L.B, Lynch, Christene, Yoshiura, S, McKinley, Ben, Dayal, P, Pindor, B, Hutter, A, Takahashi, K, Wayth, Randall, Barry, Nichole, Beardsley, A, Bowman, J, Byrne, R, Chokshi, A, Greig, B, Hasegawa, K, Hazelton, B.J, Howard, E, Jacobs, D, Kolopanis, M, Mitchell, D.A, Morales, M.F, Murray, Steven, Pober, J.C, Rahimi, M, Tingay, Steven, Webster, R.L, Wilensky, M, Wyithe, J.S.B, Zheng, Q

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A new MWA limit on the 21 cm power spectrum at redshifts ∼13-17 von Yoshiura, S, Pindor, B, Line, J.L.B, Barry, Nichole, Trott, Cathryn, Beardsley, A, Bowman, J, Byrne, R, Chokshi, A, Hazelton, B.J, Hasegawa, K, Howard, E, Greig, B, Jacobs, D, Jordan, Chris, Joseph, R, Kolopanis, M, Lynch, Christene, McKinley, Ben, Mitchell, D.A, Morales, M.F, Murray, Steven, Pober, J.C, Rahimi, M, Takahashi, K, Tingay, Steven, Wayth, Randall, Webster, R.L, Wilensky, M, Wyithe, J.S.B, Zhang, Z, Zheng, Q

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