The Space Telescope Imaging Spectrograph Design

E. Woodgate, B.; A. Kimble, Randy; Bowers, C.; B. Kraemer, S.; E. Kaiser, M.; C. Danks, A.; F. Grady, J.; J. Loiacono, J.; Brumfield, Mark; D. Feinberg, Lee; R. Gull, T.; R. Heap, Sara; P. Maran, S.; Lindler, D.; Hood, D.; Meyer, W.; VanHouten, C.; S. Argabright, Vic; Franka, Steve; L. Bybee, Richard; Dorn, David; J. Bottema, Murk; A. Woodruff, Robert; Michika, David; Sullivan, Joseph; C. Hetlinger, J.; W. Ludtke, C.; Stocker, Ralph; Delamere, A.; Rose, D.; Becker, Ignacio; Garner, H.; G. Timothy, J.; M. Blouke, Morley; L. Joseph, C.; Hartig, G.; F. Green, R.; B. Jenkins, E.; L. Linsky, Jeffrey; B. Hutchings, J.; W. Moos, H.; Boggess, A.; L. Roesler, F.; Weistrop, D.

doi:10.1086/316243

Public

The Space Telescope Imaging Spectrograph Design

Published in Publications of the Astronomical Society of the Pacific • Oct 1, 1998

Authors:

B. E. Woodgate

Randy A. Kimble

C. Bowers

Abstract

The Space Telescope Imaging Spectrograph (STIS) instrument was installed on the Hubble Space Telescope ( HST ) during the second servicing mission, in 1997 February. Four bands cover the wavelength range of 115–1000 nm, with spectral resolving powers between 26 and 200,000. Camera modes are used for...

Subject

Spectrograph

Optics

Physics

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