UV-grating performance in the High-Resolution Spectrograph.

Details UV-grating performance in the High-Resolution Spectrograph. UV-grating performance in the High-Resolution Spectrograph.

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984spie..445..436b&link_type=abstract

Instrumentation in astronomy V, p. 436 - 444

Astronomy and Astrophysics

Astronomy

2

Space Telescope:Spectrographs, Spectrographs:Space Telescope

Scientific paper

The High-Resolution Spectrograph (HRS) covers the 105 nm to 320 nm wavelength range at nominal spectral resolutions 103, 104 and 105. It employs one ruled, plane, first-order grating, four holographic, plane, first-order gratings, one r/2 echelle and two ruled, multi-partite, concave cross dispersers. The authors discuss each of the gratings individually. They review the efficiency, the measured spectral resolution, as compared to theoretical data, and also some peculiarities that came to light during the calibration of the HRS. They precede this with a description of the experimental techniques employed.

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