|Space Telescope Science Institute|
|COS Instrument Handbook Cycle 23|
The Cycle 18 calibration program continued the calibration and monitoring observations performed in Cycle 17, including long-term programs to monitor the sensitivity and wavelength scale of both the NUV and FUV detectors. Brief descriptions of these monitoring programs are presented in Table 12.2. Table 12.5 lists additional special calibration programs that were undertaken in Cycle 18. A comprehensive review of the Cycle 18 calibration program was published in COS ISR 2013-04 (Kriss et al. 2012).
124141 COS Observations of Geocoronal Lyman-α Emission List of exposures on the COS website2 that GOs may use to model and subtract Lyman-α
As described in Section 4.1.7, gain sag affects spectra obtained with the FUV detector. To address this problem the COS team performed studies to move the Aperture Mechanism so that the FUV spectra fell on a different part of the detector, called a lifetime position. This work was divided into three phases. Table 12.6 lists the programs that were used to determine the location of the new lifetime position, enable science at that location, and finally calibrate observations obtained there. The additional lifetime calibration program “Second COS FUV Lifetime Position: Wavelength Scales (FCAL1)” uses observations from programs 12805, 12806, and 12796.Table 12.6: Lifetime Position 2 Calibration Program