This paper fits pure-hydrogen white dwarf models to new HST STIS ultraviolet spectra and WFC3 photometry to produce 19 faint flux-calibration SEDs spanning 900 Å to 30 μm.
C., Hubeny, I., & Rauch, T
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Faint white dwarf flux standards: data and models
This paper fits pure-hydrogen white dwarf models to new HST STIS ultraviolet spectra and WFC3 photometry to produce 19 faint flux-calibration SEDs spanning 900 Å to 30 μm.