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Distinguishing N$_2$-Dominated from O$_2$-Dominated Atmospheres on Terrestrial Exoplanets with Reflected-Light Spectroscopy
Reflected-light spectra of Earth-sized exoplanets promise to probe habitability and biosignatures, but interpreting atmospheric oxygen can be challenging because $O_2$ can arise from both biological and abiotic processes. In addition, reflected-light retrievals exhibit degeneracies among atmospheric
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