Hopkins Ultraviolet Telescope Virtual Observatory Resource

Authors
  1. W.V. Dixon
  2. W.P. Blair
  3. J.W. Kruk
  4. M.L. Romelfanger
  5. MAST staff
  6. Published by
    Space Telescope Science Institute Archive
Abstract
      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.
    
Keywords
  1. Observational Astronomy
  2. Quasars
  3. Galaxies
  4. AGN
  5. Variable stars
  6. Nebulae
  7. Solar system
See also HTML
http://archive.stsci.edu/hut/
IVOA Identifier IVOID
ivo://archive.stsci.edu/hut

Access

IVOA Cone Search SCS
For use with a cone search client (e.g., TOPCAT).
http://archive.stsci.edu/hut/search.php?

History

2004-11-22T12:22:45Z
Resource record created

Contact

Name
Randy Thompson
E-Mail
archive@stsci.edu