R. C. Catura,1 R. A. Stern,1 W. Cash,2 D. L. Windt,2 J. L. Culhane,3 J. Lappington,3 K. Barnsdale3
1Lockheed Palo Alto Research Lab (United States) 2Center for Astrophysics and Space Astronomy (United States) 3Mullard Space Science Laboratory (England)
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We describe a rocket-borne X-ray Objective Grating Spectrograph designed to measure the spectra of cosmic sources in the 8 Å to 60 Å region with a spectral resolution of 100. Experience gained in fabricating the payload is discussed and preliminary performance data obtained in the laboratory and at the Marshall Space Flight Center are presented.
R. C. Catura,R. A. Stern,W. Cash,D. L. Windt,J. L. Culhane,J. Lappington, andK. Barnsdale
"X-Ray Objective Grating Spectrograph", Proc. SPIE 0830, Grazing Incidence Optics for Astronomical and Laboratory Applications, (9 August 1988); https://doi.org/10.1117/12.942183
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R. C. Catura, R. A. Stern, W. Cash, D. L. Windt, J. L. Culhane, J. Lappington, K. Barnsdale, "X-Ray Objective Grating Spectrograph," Proc. SPIE 0830, Grazing Incidence Optics for Astronomical and Laboratory Applications, (9 August 1988); https://doi.org/10.1117/12.942183