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- W2070139240 abstract "In a deep image of the SSA22 field taken through a narrowband filter NB912 installed in the Subaru/Suprime‐Cam, we have found the number density of the photometric Lyα emitter (LAE) candidates with LLyα>3×1042 erg s−1 at z = 6.5 is a factor of 3–7 smaller than that found at the same redshift in the Subaru Deep field (SDF). There is a trend that more luminous LAE candidates are fewer. If we consider a scenario that a larger neutral fraction of intergalactic hydrogen, xHI, in the SSA22 field obscures a part of Lyα emission, xHI in the SSA22 field should be about 2 times larger than that in the SDF, which is translated into xHI<0.9 in the SSA22 at z = 6.5." @default.
- W2070139240 created "2016-06-24" @default.
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- W2070139240 date "2010-01-01" @default.
- W2070139240 modified "2023-09-23" @default.
- W2070139240 title "Lyα emitters at z = 6.5 in the SSA22 field: A large-scale fluctuation of the neutral hydrogen fraction at the end of the reionizaion epoch?" @default.
- W2070139240 doi "https://doi.org/10.1063/1.3509304" @default.
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