STIS MAMA Cycle 12 Deep Wavecals

Details STIS MAMA Cycle 12 Deep Wavecals STIS MAMA Cycle 12 Deep Wavecals

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003hst..prop10031a&link_type=abstract

HST Proposal ID #10031

Physics

Hst Proposal Id #10031

Scientific paper

This program will obtain deep wavecals for the STIS Echelle modes in order to produce improved dispersions solutions. The new wavelength solution is based on a physical model of the instrument's optical elements and will supercede the empirical polynomial fit. This work is part of the STIS Calibration Enhancement project conducted at the ST-ECF. Deep wavecals are required in order to take full advantage of the new line list from the ESA -funded Pt/Cr-Ne calibration lamp project and to test the predictive power of physical instrument model of STIS. A second epoch of observations will investigate the issue of MSM repeatability.

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