SKA will enable Zeeman measurements of magnetic fields from cometary comas through Galactic structures and starburst galaxies to damped Ly-alpha systems at cosmological redshifts, with achievability tied to array assembly stages.
8 Water Masers in AGN with the SKA A
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Quantitative estimates indicate SKA-Mid can detect substantially more water masers in distant AGN, enabling larger statistical samples and studies up to cosmological distances.
citing papers explorer
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Measuring Magnetic Fields Near and Far with the SKA via the Zeeman Effect
SKA will enable Zeeman measurements of magnetic fields from cometary comas through Galactic structures and starburst galaxies to damped Ly-alpha systems at cosmological redshifts, with achievability tied to array assembly stages.
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Boosting Water Maser Studies in AGN with the SKA
Quantitative estimates indicate SKA-Mid can detect substantially more water masers in distant AGN, enabling larger statistical samples and studies up to cosmological distances.