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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 7.

Correction factor κ as a function of the number of pixels in the bin N. The dashed line represents the limit value of one as N tends to infinity.

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