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COS Instrument Handbook Cycle 23
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Cosmic Origins SpectrographInstrument Handbookfor Cycle 23 > Chapter 2: Special Considerations for Cycle 23 > 2.5 Non-Optimal Observing Scenarios

2.5
To optimize the scientific return of COS, we recommend that all observations be performed in TIME-TAG mode, employ the default wavelength-calibration procedures (i.e., TAGFLASH=YES), and with all four FP-POS positions (See Section 5.8) of each CENWAVE setting for the FUV gratings. Observers who wish to employ non-optimal observing techniques must strongly justify their observing strategy in the “Description of Observations” section of their Phase I proposal. A modest reduction in observational overheads will not normally be a sufficient justification for adopting non-optimal observing techniques. Whenever possible, observers should use the recommended techniques, even if this requires requesting additional resources in their Phase I proposal.

Cosmic Origins SpectrographInstrument Handbookfor Cycle 23 > Chapter 2: Special Considerations for Cycle 23 > 2.5 Non-Optimal Observing Scenarios

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