Echelle Blaze Shift vs. MSM Monthly Offset

Details Echelle Blaze Shift vs. MSM Monthly Offset Echelle Blaze Shift vs. MSM Monthly Offset

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002hst..prop.9619v&link_type=abstract

HST Proposal ID #9619

Physics

Hst Proposal Id #9619

Scientific paper

In the near future, monthly MSM offsets will probably be disabled for STIS echelle gratings, alleviating to some extent calibration problems associated with the monthly offsets. The data from this program will be used to improve empirical and optical models relating wavelength and blaze function shifts. These models will in turn be used to improve the calibration of archival echelle data obtained while monthly MSM offsets were enabled. The flux standard HZ43 will be observed with the E230H echelle grating at a central wavelength of 2513 Angstroms. Five exposures will be obtained, each with a different monthly offset applied to the Mode Select Mechanism {MSM}.

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