STIS MAMA Dispersion Solutions

Details STIS MAMA Dispersion Solutions STIS MAMA Dispersion Solutions

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002hst..prop.9618v&link_type=abstract

HST Proposal ID #9618

Computer Science

Performance

Hst Proposal Id #9618

Scientific paper

Obtain wavecals just deep enough to constrain wavelength and spatial distorion maps without overusing the calibration lamp. For the first time on orbit, data will be obtained at all available central wavelengths. This information will help constrain global models of STIS optical performance being developed at ECF and STScI. During the observations, MSM monthly offsets will be set to zero to complement observations over the past couple of cycles, which occured at extreme monthly offsets. The echelle observations at zero offset will yield dispersion solutions that are directly applicable to all echelle science data obtained after monthly offsets are disabled.

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