UVES data identify 6-14 HI absorbers per halo with N_HI from 10^12 to 10^17 cm^-2, 70% spatially resolved along the jet with little column density change over >30 kpc, and JWST shows a kinematic link to [OIII] outflows suggesting common origin.
The Lyαparameters and uncertainties are derived from the posterior distributions of the MCMC sampling
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Exploring the gaseous halos of z>3 radio galaxies with UVES and JWST/NIRSpec
UVES data identify 6-14 HI absorbers per halo with N_HI from 10^12 to 10^17 cm^-2, 70% spatially resolved along the jet with little column density change over >30 kpc, and JWST shows a kinematic link to [OIII] outflows suggesting common origin.