STScI

Cosmic Origins Spectrograph Instrument Handbook for Cycle 17

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5.5 FUV gap coverage and single segment usage


The FUV detector contains two segments whose active areas are separated by a gap approximately 9 mm wide. The optical image of the spectrum is continuous, but the wavelengths that fall on the gap are not recorded. The area between the two segments of the FUV detector causes an 18-20 Å gap in the wavelength coverage for the G130M and G160M gratings, for example. Depending upon the science requirements of the observation, these wavelengths can be brought onto the active area of the detector by choosing one of the alternate central wavelength settings. Each FUV "M" grating has five central wavelength settings and the G140L has two. Wavelengths that fall on the gap with one of the settings are visible with at least one of the others.

Single segment usage

The COS FUV detector consists of two distinct segments which are, at the lowest commanding level, operated and read out independently. Normally, both detector segments are utilized for a science exposure, however, there are circumstances where operating with one detector segment at the nominal high voltage and the other effectively turned off may be beneficial. The SEGMENT Optional Parameter allows this choice. STScI strongly recommends usage of both segments (the default for all but the G140L 1105 Å setting) unless very special circumstances exist. Such circumstances include, but are not limited to:

Wavelength and flat-field calibration procedures will remain the same for a particular segment whether the other segment is operating or not.

The Optional Parameter SEGMENT (=BOTH (default), A, or B) specifies which segment of the FUV detector to use for an observation. A value of BOTH will activate both segments. If A is selected, only segment A of the detector will be activated for photon detection, and the spectrum will contain data from only that half of the detector. If B is selected, only segment B of the detector will be activated and used to generate data.

If grating G140L is specified with the 1105 Å wavelength setting, then the value must be A. Bear in mind that segment A detects the longer wavelength light and segment B the shortest wavelengths, and this is true for all FUV settings.


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