Space Telescope Imaging Spectrograph Instrument Handbook for Cycle 17

17.5 Cycle 8 Calibration

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The Cycle 8 calibration plan was modeled closely on the Cycle 7 calibration plan. Once again, supported modes were monitored for such things as sensitivity changes, flat field evolution, and dispersion solutions. No additional calibrations were taken for most available-but-unsupported configurations.

In addition to monitoring instrument health and safety and maintaining the overall calibration of STIS supported modes, our special goals were as follows:

1. To improve the imaging throughput calibration accuracy (to better than the current 5% systematic uncertainty);
2. To improve PSF characterization in imaging mode and in coronagraphic mode;
3. To improve CCD hot pixel and bias subtraction;
4. To improve the CCD charge transfer efficiency (CTE) characterization for sparse fields at low count levels;
5. To calibrate the dispersion as a function of position for MAMA slitless spectroscopy with the L-mode gratings;
6. To characterize observations with the FUV-MAMA repeller wire turned off, with the aim of possibly making this available for Cycle 10. This should improve the spectral resolution at the expense of a ~35% loss of sensitivity.

The results of all the Cycle 8 calibration programs are presented in the close-out report STIS ISR 2001-04.