SKAO will enable HI and OH absorption surveys to characterize cold gas properties in galaxies from z=0 to beyond z=6.
and Pandey-Pommier, M and Roy, Nirupam and others , title =
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The paper reviews the potential of SKA-VLBI for parsec-scale HI 21-cm imaging in molecular gas-rich radio AGN to study jet-ISM interactions and AGN feedback.
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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Tracing Cold Gas in Absorption Across Cosmic Time with the SKA
SKAO will enable HI and OH absorption surveys to characterize cold gas properties in galaxies from z=0 to beyond z=6.
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Uncovering neutral Hydrogen clouds in Radio Galaxies in the SKA era
The paper reviews the potential of SKA-VLBI for parsec-scale HI 21-cm imaging in molecular gas-rich radio AGN to study jet-ISM interactions and AGN feedback.
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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.