Abstract
In the next 10–20 years, several observatories will aim to detect the signatures of oxygenic photosynthesis on exoplanets, though targets must be carefully selected. Most known potentially habitable exo-planets orbit cool M-dwarf stars, which have limited emission in the photosynthetically active region of the spectrum (PAR, 400
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Chitnavis, S., Gray, C., Rousouli, I., Gillen, E., Mullineaux, C. W., Haworth, T. J., & Duffy, C. D. P. (2024). Optimizing photosynthetic light-harvesting under stars: simple and general antenna models. Photosynthesis Research, 162(1), 75–92. https://doi.org/10.1007/s11120-024-01118-1
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