STScI

Cosmic Origins Spectrograph Instrument Handbook for Cycle 17

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6.4 TIME-TAG or ACCUM?


Most of the considerations regarding TIME-TAG and ACCUM exposures for NUV imaging are the same as for NUV spectroscopy; the reader is referred to Chapter 5 for a discussion. One difference is that, in contrast to spectroscopy in ACCUM mode, no doppler correction is performed on the events in imaging mode.

We caution that particular attention should be given to the expected count rate, since imaging mode is efficient and can lead to high count rates compared to spectroscopic observations.


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