Fig. 2

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Exoplanet detections around giant stellar hosts (log g < 3.5 cm s−2) from the NASA Exoplanet archive. Circles are color-coded as a function of the detection method (blue for RV and brown for transit). Yellow stars represent the targets published by Ottoni et al. (2022) and Pezzotti et al. (2022), and red stars the targets of this study.
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