Hopkins Ultraviolet Telescope

The Hopkins Ultraviolet Telescope (HUT) was a shuttle-borne instrument used to obtain ultraviolet spectra in the far ultraviolet region of the spectrum. It was part of the ASTRO payload complement of three co-mounted instruments that flew in December 1990 and March 1995 as Space Shuttle missions. More than 650 spectra were obtained of 340 targets. In April, 2013, the HUT data was reprocessed to improve calibration, expand metadata, add new data products, and update file formats. The current cone service uses the metadata from these reprocessed files.

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/archive.stsci.edu/hut
Related Identifier http://archive.stsci.edu/hut/
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://archive.stsci.edu/hut
Provenance
Creator W.V. Dixon; W.P. Blair; J.W. Kruk; M.L. Romelfanger; MAST staff
Publisher Space Telescope Science Institute Archive
Publication Year 2004
OpenAccess true
Contact Randy Thompson <archive(at)stsci.edu>
Representation
Resource Type Other; AstroObjects
Discipline Astrophysics and Astronomy; Galactic and extragalactic Astronomy; High Energy Astrophysics; Interstellar medium; Natural Sciences; Observational Astronomy; Physics; Solar System Astronomy; Stellar Astronomy