NISER-IUCAA New Simulations of JWST GAlaxies and Quasars(NINJA): Properties of galaxies at
The NINJA suite of cosmological hydrodynamical simulations demonstrates that while specific spectral and dust models can reproduce observed UV luminosity functions for galaxies at , significant degeneracies between feedback and dust properties, along with resolution limitations at , necessitate higher-resolution simulations and multi-wavelength observations to robustly constrain high-redshift galaxy evolution.