Spectroscopic monitoring detects phase-locked flares to Proxima d and flare-intensity modulation by Proxima b, producing a -16 G polar field estimate for the inner planet via Poynting-flux modeling.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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Four transiting sub-Neptunes with radii measured to <1.7% precision and masses >3 sigma for three planets, plus an outer non-transiting companion, discovered around TOI-5624 via TESS, CHEOPS photometry, and ground-based RV data.
A new discrete-time autoregressive model (CIAR) is proposed for irregular time series; it is shown to be weakly stationary, admits a state-space representation for Kalman estimation, and is applied to stellar light curves for model checking and forecasting.
citing papers explorer
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Star-planet interaction in the Proxima system
Spectroscopic monitoring detects phase-locked flares to Proxima d and flare-intensity modulation by Proxima b, producing a -16 G polar field estimate for the inner planet via Poynting-flux modeling.
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The multi-planet system TOI-5624: Four transiting sub-Neptunes with an outer companion revealed by transit-timing variations
Four transiting sub-Neptunes with radii measured to <1.7% precision and masses >3 sigma for three planets, plus an outer non-transiting companion, discovered around TOI-5624 via TESS, CHEOPS photometry, and ground-based RV data.
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Discrete-time autoregressive model for unequally spaced time-series observations
A new discrete-time autoregressive model (CIAR) is proposed for irregular time series; it is shown to be weakly stationary, admits a state-space representation for Kalman estimation, and is applied to stellar light curves for model checking and forecasting.