volume 12, issue S333, P292-295 2017
DOI: 10.1017/s1743921317011152
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Shintaro Yoshiura, Jack L. B. Line, Kenji Kubota, Kenji Hasegawa, Keitaro Takahashi

Abstract: AbstractThe cross power spectrum of the 21 cm signal and Lyman-α emitters (LAEs) is a probe of the Epoch of Reionization. Astrophysical foregrounds do not correlate with the LAE distribution, though the foregrounds contribute to the error. To study the impact of foregrounds on the measurement, we assume realistic observation by the Murchison Widefield Array using a catalogue of radio galaxies, a LAE survey by the Subaru Hyper Supreme-Cam and the redshift of LAEs is determined by the Prime Focus Spectrograph. T…

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