Forecasts indicate SKA-Mid AA4 will measure the HI power spectrum at high significance from z~1 to z~3 near k~1 Mpc^{-1}, extending MeerKAT results to constrain HI galaxy properties and galaxy evolution.
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4 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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UNVERDICTED 4representative citing papers
An update to a prior SKA HI science chapter that restates and adjusts a three-tiered survey strategy for mapping atomic hydrogen morphologies, kinematics, and cosmic density evolution.
Review of HI gas studies, cosmic web processes, and SKA's role in advancing the field through high-sensitivity surveys.
Optical spectroscopy is required to unlock the full potential of SKAO extragalactic surveys through precise redshifts, activity diagnostics, HI stacking, and large-scale structure mapping.
citing papers explorer
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Interferometric HI Intensity Mapping of the Late Time Universe with SKA-Mid
Forecasts indicate SKA-Mid AA4 will measure the HI power spectrum at high significance from z~1 to z~3 near k~1 Mpc^{-1}, extending MeerKAT results to constrain HI galaxy properties and galaxy evolution.
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HI Galaxy Science with the SKA
An update to a prior SKA HI science chapter that restates and adjusts a three-tiered survey strategy for mapping atomic hydrogen morphologies, kinematics, and cosmic density evolution.
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Studying HI and the Cosmic Web in the Era of SKA
Review of HI gas studies, cosmic web processes, and SKA's role in advancing the field through high-sensitivity surveys.
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Unlocking the Full Potential of SKAO Extra-galactic Science with High-multiplex Optical Spectroscopy
Optical spectroscopy is required to unlock the full potential of SKAO extragalactic surveys through precise redshifts, activity diagnostics, HI stacking, and large-scale structure mapping.