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Constraining the 21cm 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. Howard,D. 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

Monthly Notices of the Royal Astronomical Society（2021）

Cited 4|Views45
Key words
instrumentation: interferometers,methods: statistical
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