Paper
28 July 2000 Calibrations and flight performance of the extreme ultraviolet opacity rocket
Author Affiliations +
Abstract
A sounding rocket observation of G191-B2B, a hot white dwarf star, was made on 27 September 1999 over a wavelength range of 220 - 340 angstroms with the Extreme ultraviolet Opacity Rocket (EOR), an EUV spectrograph. EOR acquired over 200 seconds of data above 200 km. Two broadband multilayer- coated diffraction gratings in Wadsworth mounts provide EOR with a peak effective area of 2.5 cm2 near 280 angstroms and spectral resolution of (lambda) /(Delta) (lambda) equals 2500 - 3000. Preliminary examination of the flight spectrum suggests the presence of absorption features which are not apparent in lower resolution spectra.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Kurt S. Gunderson, Erik Wilkinson, and James C. Green "Calibrations and flight performance of the extreme ultraviolet opacity rocket", Proc. SPIE 4013, UV, Optical, and IR Space Telescopes and Instruments, (28 July 2000); https://doi.org/10.1117/12.394024
Lens.org Logo
CITATIONS
Cited by 2 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Extreme ultraviolet

Calibration

Spectrographs

Sensors

Rockets

Opacity

Stars

Back to Top