Detection of hydrocarbons in Titan using high-resolution cross-correlation spectroscopy

arXiv:2609.03975 · astro-ph.EP, astro-ph.IM, astro-ph.SR, physics.ao-ph, physics.space-ph · Submitted 2026-09-03 · Read on arXiv

astro-ph.EP, astro-ph.IM, astro-ph.SR, physics.ao-ph, physics.space-ph

Submitted: 2026-09-03

Updated: 2026-09-03

Code: https://github.com/ExoMol/ExoCross

Terminology

Calibration — 10× in this paper · explained in 7 episodes
Fidelity — 7× in this paper · explained in 2 episodes
Degeneracy — 6× in this paper · explained in 3 episodes
Abundance — 4× in this paper · explained in 1 episode
Accuracy — 3× in this paper · explained in 1 episode
Trace — 3× in this paper · explained in 2 episodes
Benchmark — 2× in this paper · explained in 2 episodes
ESO Very Large Telescope — 2× in this paper
Extremely Large Telescope — 2× in this paper
Metallicity — 2× in this paper · explained in 3 episodes
Signal-to-noise ratio (SNR) — 2× in this paper · explained in 2 episodes
Ab Initio — 1× in this paper · explained in 1 episode
Ablation — 1× in this paper · explained in 1 episode
Absorption Cross Section — 1× in this paper · explained in 1 episode
Adam — 1× in this paper · explained in 2 episodes
Alignment — 1× in this paper · explained in 1 episode
Consistency — 1× in this paper · explained in 3 episodes
Robustness — 1× in this paper · explained in 5 episodes
Transmission spectroscopy — 1× in this paper · explained in 2 episodes
Voyager and the Infrared Space Observatory — 1× in this paper

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