Earth Analogs in Reflected Light: Insights from Early Spectral Characterization in Unconstrained Orbits
Arnaud Salvador, Tyler D. Robinson

TL;DR
This study evaluates how different spectral bandpasses and S/N levels affect the ability of space-based observatories to characterize Earth-like exoplanets using reflected light spectroscopy, emphasizing the importance of spectral coverage.
Contribution
It introduces a framework for assessing the spectral and S/N requirements for retrieving planetary parameters from early spectral data of Earth analogs.
Findings
Broader spectral coverage enhances parameter retrieval.
Limited spectral bands can still provide significant information at moderate S/N.
Combining visible and NIR ranges yields the most comprehensive characterization.
Abstract
A next generation of space-based observatories aims to detect and characterize potentially Earth-like exoplanets around Sun-like stars using reflected light spectroscopy. However, it remains unclear how such direct imaging observationslimited in spectral coverage and signal-to-noise ratio (S/N)translate into constraints on atmospheric composition and habitability. Coronagraphs used for high-contrast imaging typically operate over narrow bandpasses, and exposure time limits can restrict data quality. To optimize observing strategies and instrument design, we use our atmospheric retrieval tool, , to assess the performance of a -type mission across different spectral bandpasses ("Red", "Blue", "Visible", "NIR", and their combination) and S/N levels (10, 15, and 20; from moderate to moderate-high observation quality) in…
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