A far ultraviolet rocket-borne spectrograph |
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Authors: | Webster Cash Timothy Cook Clarke Chambellan Donald Heyse David Hofmockel Theodore P Snow David Windt Clyde Zaidins |
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Institution: | (1) Center for Astrophysics and Space Astronomy, University of Colorado, 80309-0391 Boulder, CO, USA;(2) Present address: Department of Astrophysical, Planetary and Atmospheric Sciences, Boulder, USA;(3) Present address: AT&T Bell Laboratories, Murray Hill, NJ, USA;(4) Present address: Department of Physics, University of Colorado, Denver, USA |
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Abstract: | A sensitive spectrograph for rocket observations of celestial objects in the 910–1250Å band is described. The instrument incorporates a variety of new technologies that allow unprecedented sensitivity in this difficult, but scientifically rewarding, band. It includes a diamond-turned Wolter-Schwarzschild Type II telescope, a conventional Rowland Circle spectrograph, and resistive anode/micro-channel plate detectors. It has been launched twice from Woomera, Australia where it performed the only observations of SN1987a in its bandpass and discovered a new feature in the diffuse ultraviolet background. |
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