Strong-feedback models with bright galaxies match JWST UVLF at z greater than or equal to 10 and predict an extended reionization from z approximately 16 to 6 that fits CMB optical depth within 2 sigma.
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Setting the cold neutral medium density to 7500 cm^{-3} in a model for MACS0416_Y1 allows UV trapping and reduced supernova destruction, reproducing the UV-to-FIR SED with intermediate-size grains dominating the infrared output.
citing papers explorer
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Towards Reconciling Reionization with JWST: The Role of Bright Galaxies and Strong Feedback
Strong-feedback models with bright galaxies match JWST UVLF at z greater than or equal to 10 and predict an extended reionization from z approximately 16 to 6 that fits CMB optical depth within 2 sigma.
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Resolving the Dust Budget Crisis at $z \sim 8$ with Optically Thick, High-Density Molecular Clumps: MACS0416_Y1
Setting the cold neutral medium density to 7500 cm^{-3} in a model for MACS0416_Y1 allows UV trapping and reduced supernova destruction, reproducing the UV-to-FIR SED with intermediate-size grains dominating the infrared output.