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

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

Internet

http://purl.org/au-research/grants/arc/CE170100013
http://hdl.handle.net/20.500.11937/91574

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