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Calamida, A · 2022

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astro-ph.IM 1

years

2024 1

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CONDITIONAL 1

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Faint white dwarf flux standards: data and models

astro-ph.IM · 2024-11-13 · conditional · novelty 5.0

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.

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  • Faint white dwarf flux standards: data and models astro-ph.IM · 2024-11-13 · conditional · none · ref 8

    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.