GHRS Ech-B Sensitivity - 4

Details GHRS Ech-B Sensitivity - 4 GHRS Ech-B Sensitivity - 4

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.5597h&link_type=abstract

HST Proposal ID #5597

Physics

Hst Proposal Id #5597 Calibration

Scientific paper

This proposal defines a series of observations that will reestablish the sensitivity calibration of the GHRS Echelle B spectroscopic mode during cycle 4. It makes use of the UV standard star Mu Columbae, with target acquisitions performed using mirror A2. The OSCAN mode is used to scan orders 18-31 at three carrousel positions that straddle the peak of the blaze function, with the star in the LSA. Only the peak of blaze will be scanned with the star in the SSA.

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