At IAS, I developed a Bayesian MCMC approach to analyze infrared spectra from NASA’s Perseverance rover. By coupling radiative transfer modeling with advanced optimization, I improved mineralogical fits and quantified uncertainties—gaining hands-on experience at the crossroads of planetary science, numerical methods, and space exploration.
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During summer 2024 (June 3 – August 30, 2024), I completed a research internship as an assistant engineer within the Planetology team at the IAS (Institut d’Astrophysique Spatiale), under the supervision of Dr. François Poulet and Dr. Clément Royer. My work was part of the Mars 2020 mission: I focused on data from the passive infrared spectrometer IRS / SuperCam onboard the Perseverance rover, with the objective of improving the reflectance spectra fitting procedure in order to estimate mineralogy (abundances, grain sizes) and—most importantly—quantify the uncertainties associated with inferred parameters.
The core of the project was to couple a radiative transfer model (Shkuratov model) with a Bayesian optimization procedure (MCMC) to extract parameter distributions from Martian spectra. My tasks combined numerical optimization (improving a simplex / Nelder-Mead method), implementation and testing of MCMC samplers (affine-invariant ensemble sampler), and systematic validation on laboratory spectra before applying the approach to Martian targets.
This internship was a valuable immersion in space research, allowing me to bridge advanced numerical methods with real scientific questions (uncertainty quantification, robustness of inferences). The experience confirmed my intention to pursue a Master’s in Astrophysics and gave me concrete ideas for extending this work (further optimization of the MCMC algorithm, extended validation, contribution to instrument calibration).
Download the full internship report for in-depth
technical documentation and detailed findings.