Five new HI 21-cm absorption detections in LERGs and HERGs at z<0.5 reveal disturbed gas kinematics with velocity offsets over 350 km/s and a 3% detection rate consistent with lower-redshift samples.
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Low-frequency radio recombination lines observable with the SKA will enable multi-phase gas studies in galaxies and AGN from z~0 to z~6, probing the HI-to-H2 transition, diffuse ionized gas, and compact AGN environments.
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HI 21-cm absorption in low- and high-excitation radio-loud AGNs at $z<0.5$ from MALS
Five new HI 21-cm absorption detections in LERGs and HERGs at z<0.5 reveal disturbed gas kinematics with velocity offsets over 350 km/s and a 3% detection rate consistent with lower-redshift samples.
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Low-Frequency Recombination Lines from Galaxies and AGN over Cosmic Time
Low-frequency radio recombination lines observable with the SKA will enable multi-phase gas studies in galaxies and AGN from z~0 to z~6, probing the HI-to-H2 transition, diffuse ionized gas, and compact AGN environments.