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Faint Object Spectrograph
The Faint Object Spectrograph (FOS) was one of the 4 original axial instruments aboard the Hubble Space Telescope (HST). The FOS was designed to make spectroscopic observations of astrophysical sources from the near ultraviolet to the near infrared (1150 - 8000 Angstroms). The instrument was removed from HST during the Second Servicing Mission in February 1997.
Complete Metadata
| bureauCode |
[ "026:00" ] |
|---|---|
| identifier | ivo://archive.stsci.edu/hst/fos |
| landingPage | http://www.stsci.edu/hst/fos |
| programCode |
[ "026:000" ] |
| theme |
[ "Astrophysics" ] |
