Search Results - Line, J.L.B.

A new MWA limit on the 21 cm power spectrum at redshifts ∼13-17 by 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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Constraining the 21 cm brightness temperature of the IGM at z = 6.6 around LAEs with the murchison widefield array by 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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