Efficiency functions for a 316 g/mm echelle grating

Details Efficiency functions for a 316 g/mm echelle grating Efficiency functions for a 316 g/mm echelle grating

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986spie..627..395c&link_type=abstract

IN: Instrumentation in astronomy VI; Proceedings of the Meeting, Tucson, AZ, Mar. 4-8, 1986. Part 1 (A87-36376 15-35). Bellingha

Astronomy and Astrophysics

Astronomy

1

Echelle Gratings, Radiometric Resolution, Transmission Efficiency, Angular Resolution, Calibrating, High Resolution, Hubble Space Telescope, Incidence, Spectrographs

Scientific paper

The radiometric response function of the High Resolution Spectrograph (HRS) for the Hubble Space Telescope was measured in 1984. From the system efficiency measurements made in the HRS echelle modes, the relative efficiencies ('ripple' functions) of 14 HRS echelle orders have been deduced. The results agree well with a theoretical model of echelle efficiency, except for a residual shift of apparent blaze angle with spectral order. The discrepancy between nominal and fitted blaze angle decreases with increasing order number.

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