Impacts of high-contrast image processing on atmospheric retrievals
Evert Nasedkin, Paul Molli\`ere, Jason Wang, Faustine Cantalloube,, Laura Kreidberg, Laurent Pueyo, Tomas Stolker, Arthur Vigan

TL;DR
This study investigates how high-contrast image processing algorithms affect the spectral data of exoplanets and demonstrates that accounting for wavelength correlations improves the accuracy of atmospheric parameter retrievals.
Contribution
The paper systematically analyzes the impact of different image processing algorithms on spectral retrieval accuracy and emphasizes the importance of including wavelength covariance in Bayesian atmospheric retrievals.
Findings
Choice of processing algorithm significantly affects retrieval bias.
Including full covariance matrix improves parameter accuracy.
Full covariance inclusion is statistically favored in retrievals.
Abstract
Many post-processing algorithms have been developed in order to better separate the signal of a companion from the bright light of the host star, but the effect of such algorithms on the shape of exoplanet spectra extracted from integral field spectrograph data is poorly understood. The resulting spectra are affected by noise that is correlated in wavelength space due to both optical and data processing effects. Within the framework of Bayesian atmospheric retrievals, we aim to understand how these correlations and other systematic effects impact the inferred physical parameters. We consider three algorithms (KLIP, PynPoint and ANDROMEDA), optimizing the choice of algorithmic parameters using a series of injection tests into archival SPHERE and GPI data of the HR 8799 system. The wavelength-dependent covariance matrix is calculated to provide a measure of instrumental and algorithmic…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Spectroscopy and Chemometric Analyses · Blind Source Separation Techniques
