  The Hopkins Ultraviolet Telescope (HUT) was a 0.9 m telescope and
moderate-resolution (~3 A) far-ultraviolet (820-1850 A) spectrograph that flew
twice on the space shuttle, in 1990 December (Astro-1, STS-35) and 1995 March
(Astro-2, STS-67). The resulting spectra were originally archived in a
non-standard format that lacked important descriptive metadata. To increase
their utility, we have modified the original data-reduction software to produce
a new and more user-friendly data product, a time-tagged photon list similar in
format to the Intermediate Data Files (IDFs) produced by the {\it Far
Ultraviolet Spectroscopic Explorer} calibration pipeline. We have transferred
all relevant pointing and instrument-status information from locally-archived
science and engineering databases into new FITS header keywords for each data
set. Using this new pipeline, we have reprocessed the entire HUT archive from
both missions, producing a new set of calibrated spectral products in a modern
FITS format that is fully compliant with Virtual Observatory requirements. For
each exposure, we have generated quick-look plots of the fully-calibrated
spectrum and associated pointing history information. Finally, we have
retrieved from our archives HUT TV guider images, which provide information on
aperture positioning relative to guide stars, and converted them into
FITS-format image files. All of these new data products are available in the
new HUT section of the Mikulski Archive for Space Telescopes (MAST), along with
historical and reference documents from both missions. In this paper, we
document the improved data-processing steps applied to the data and show
examples of the new data products.
