Fig. 4.

Illustration of the model grid from Sect. 5. The plot shows the effective temperature Teff and the photospheric density ρph for all atmosphere models. At low temperatures the actual photospheric density can exceed the targeted upper limit of 8 × 10−14 g cm−3, due the development of a strong recombination wave, which complicates the mapping between photospheric properties and the computational grid.
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