| Space Telescope Science Institute |
| COS Instrument Handbook |
| help@stsci.edu |
The Cycle 19 calibration program continued the routine calibration and monitoring observations performed in Cycle 18, including long-term programs to monitor the sensitivity and wavelength scale of both the FUV and NUV detectors. Brief descriptions of these programs are listed in Table 12.5.Table 12.5: Cycle 19 Calibration Program
S/N = 20–25 per 3×3 pixel element None1 COS Observations of Geocoronal Lyman α Emission