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- W3105461770 abstract "We investigate the potential use of nebular emission lines in the rest-frame far-infrared (FIR) for determining spectroscopic redshift of z > 8 galaxies with the Atacama Large Millimeter/submillimeter Array (ALMA). After making a line emissivity model as a function of metallicity, especially for the [O iii] 88 μm line which is likely to be the strongest FIR line from H ii regions, we predict the line fluxes from high-z galaxies based on a cosmological hydrodynamics simulation of galaxy formation. Since the metallicity of galaxies reaches at ∼0.2 Z☉ even at z > 8 in our simulation, we expect the [O iii] 88 μm line as strong as 1.3 mJy for 27 AB objects, which is detectable at a high significance by <1 hr integration with ALMA. Therefore, the [O iii] 88 μm line would be the best tool to confirm the spectroscopic redshifts beyond z = 8." @default.
- W3105461770 created "2020-11-23" @default.
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- W3105461770 date "2013-12-16" @default.
- W3105461770 modified "2023-10-02" @default.
- W3105461770 title "ALMA WILL DETERMINE THE SPECTROSCOPIC REDSHIFT <i>z</i> > 8 WITH FIR [O III] EMISSION LINES" @default.
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- W3105461770 doi "https://doi.org/10.1088/2041-8205/780/2/l18" @default.
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