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List of Figures
The Astro Observatory mounted in the shuttle
Line drawing of HUT instrument
Location of the hardware used to attach telescopes to IPS
The principal elements contained within the ECC
The HUT primary mirror
The HUT spectrometer system
Intensified photodiode array detector
Display: HOP HUT Operations
Display: HDC HUT doors and camera
Display: HMH HUT mirror and heater
HUT Astro-1 Lyman-
scattering profile
Flat field correction for the small aperture door
Raw counts spectrum of G191-B2B
HUT inflight/postflight calibration comparison
Expected 2nd order effective area for Astro-2
Expected 2nd order + Al filter effective area for Astro-2
Extended source sensitivity for S/N = 10 per Å
HUT airglow,
20'' aperture, Day, 1800 s
6/23/1999