Transmission spectra for the warm Saturn HATS-6b for λ = 0.3 μm to 25 μm including the total spectrum of the final iteration (iteration 5) and the morning and evening terminator separately. We also show the contributions of selected gas-phase species, the contribution of the Si-bearing cloud particle materials, and the spectral accuracy of the JWST instruments NIRSpec prism and MIRI LRS for two and ten transits.