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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 4.

Gap histogram for different cases. Real data from 2006 January 15 (solid dark line) are shown alongside the best fit (red solid line). A histogram is created in the 1600–1850 Å range in the FUV channel where no signal other than noise is identified. The dotted and dashed lines are presented to illustrate the effect of changing the initial count in the model.

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