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Synthetic Photometry
Model:
Levenhagen 2017
A grid of LTE and non-LTE synthetic spectra of hot DA white dwarfs. It covers Teff from 17,000 K to 100,000 K and log(g) from 7.0 to 9.5. The stellar models are built for pure hydrogen and the spectra cover a wavelength range from 90 nm to 2.5 micron.
Model parameters
Teff: - (?)
Logg: - (?)

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