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

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

The locations of Ly α-emitting galaxies (LAEs) at the end of the Epoch of Reionization (EoR) are expected to correlate with regions of ionized hydrogen, traced by the redshifted 21 cm hyperfine line. Mapping the neutral hydrogen around regions with detected and localized LAEs offers an avenue to con...

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Bibliographic Details
Main Authors:	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.
Format:	Journal Article
Language:	English
Published:	OXFORD UNIV PRESS 2021
Subjects:	Science & Technology Physical Sciences Astronomy & Astrophysics instrumentation: interferometers methods: statistical LY-ALPHA EMITTERS OPACITY FLUCTUATIONS REIONIZED BUBBLES GALAXY FORMATION EPOCH REDSHIFT TOPOLOGY ISLANDS SIZES astro-ph.CO astro-ph.IM
Online Access:	http://purl.org/au-research/grants/arc/CE170100013 http://hdl.handle.net/20.500.11937/91574

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