Calibrated First-Order HUT Spectra of White Dwarfs G191-B2B and HZ 43 ("HUT-WDS")

During the Astro-1 mission, an aluminum filter was used to block first-order light, and two white dwarfs (G191-B2B and HZ 43) were observed in second order. The flux from these second-order observations were then subtracted from the first-order spectra of these two objects. This was the only time that such second-order corrections were applied to HUT spectra, because no second-order observations were obtained during Astro-2. Because these spectra are in a different format compared to the rest of the HUT data products on MAST, they are provided here as an HLSP.