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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 9.

Limb radiance and the associated standard error, integrated between 1600 and 1900 Å to probe haze scattering. This altitude profile corresponds to the limb above Titan’s equator on 2006 January 15. Brown dots are the evening limb, blue ones are the morning limb. Individual pixel radiances are shown as an error bar corresponding to their integrated uncertainty.

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