GHRS G140M Sensitivity and Vignetting CALIBRATION--CYCLE5

Details GHRS G140M Sensitivity and Vignetting CALIBRATION--CYCLE5 GHRS G140M Sensitivity and Vignetting CALIBRATION--CYCLE5

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995hst..prop.6212s&link_type=abstract

HST Proposal ID #6212

Physics

Hst Proposal Id #6212 Calibration

Scientific paper

This proposal defines a series of observations that will reestablish the sensitivity calibration of the GHRS G140M A spectroscopic mode during cycle 4. It makes use of the UV standard star Mu Columbae, with target acquisitions performed using mirror A1. The WSCAN mode is used to scan wavelengths between 1100A and 1600A. At shorter wavelengths the COSTAR coatings are expected to absorb most of the light. At longer wavelengths either G160M or G200M may be used instead of G140M. Both the LSA and the SSA will be calibrated.

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