Echelle Grating Blaze Function Zero Points

Details Echelle Grating Blaze Function Zero Points Echelle Grating Blaze Function Zero Points

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008hst..prop11866a&link_type=abstract

HST Proposal ID #11866. Cycle 17

Computer Science

Scientific paper

We will observe the flux standard G191B2B,obtaining echelle spectra in all primary and intermediate wavelength settings. While this was done in cycle 10 {8915}, the echelle blaze shift has proved to depend sensitively on side of operation, time and the exact MSM positioning. We therefore believe it is important to obtain a complete set of post-repair data at default MSM position to allow a comprehensive solution for the echelle blaze shifts on a repaired side 2.;

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