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Methods for Analysing Low Signal-to-noise-ratio Emission Observations: The Cassini Ultraviolet Imaging Spectrograph Pipeline and Application to Titan Airglow Observations

  • Authors: Nathan Le Guennic, Panayotis Lavvas, Tommi Koskinen, Devin Hoover

Nathan Le Guennic et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 5.

Raw spectrum (orange bars) of pixel 50 on exposure 26 of Titan flyby T10. A large part of the spectrum has zero counts, which is statistically unphysical. For comparison, a typical raw spectrum is shown in dark blue bars upside down.

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