| Cosmic Origins Spectrograph Instrument Handbook for Cycle 17 | ||||
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6.5 Attenuation Considerations
As mentioned at the beginning of this chapter, there are two instrument parameters which must be specified for imaging:
PSAorBOA, andMIRRORAorMIRRORB. With attenuation factors of 100 and 25 respectively,BOAandMIRRORBallow one to observe a large dynamic range of target fluxes. For example, the imaging exposure time calculator indicates that a target with a flat spectrum of 1 FEFU will give a total source count rate of 263 counts sec-1, and a rate of about 26 counts sec-1 in the brightest pixel, using thePSAandMIRRORA. These are both well within acceptable NUV detector safety limits. With theBOA, one could image a target with a flux of 100,000 FEFU at the same count rate. With both theBOAandMIRRORB, the flux becomes 2.5 × 106 FEFU.
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