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The EBLM Project– XI. Mass, radius, and effective temperature measurements for 23 M-dwarf companions to solar-type stars observed with CHEOPS
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Closeby Habitable Exoplanet Survey (CHES). I. Astrometric Noise and Planetary Detection Efficiency Due to Stellar Spots and Faculae
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Predicting Solar cycle 25 using an optimized long short-term memory model based on sunspot area data
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Improving exoplanet detection power: Multivariate Gaussian process models for stellar activity
A non-linear approach to predicting the amplitude and timing of the sunspot area in cycle 25
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A New Method for Estimating Starspot Lifetimes Based on Autocorrelation Functions
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Average annual total sunspot area in the last 410 yr: the most probable values and limits of their uncertainties
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Forward modelling of Kepler-band variability due to faculae and spots
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Prediction of Amplitude and Timing of Solar Cycle 25
Solar observatory Einstein Tower: Data release of the digitized solar full‐disk photographic plate archive
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Amplification of Brightness Variability by Active-region Nesting in Solar-like Stars
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Toward Extremely Precise Radial Velocities. I. Simulated Solar Spectra for Testing Exoplanet Detection Algorithms
Reconstruction of spectral solar irradiance since 1700 from simulated magnetograms
M. Dasi-Espuig, J. Jiang, N. A. Krivova, et al. Astronomy & Astrophysics 590 A63 (2016) https://doi.org/10.1051/0004-6361/201527993
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Stellar activity as noise in exoplanet detection – I. Methods and application to solar-like stars and activity cycles
H. Korhonen, J. M. Andersen, N. Piskunov, et al. Monthly Notices of the Royal Astronomical Society 448(4) 3038 (2015) https://doi.org/10.1093/mnras/stu2730
A homogeneous database of sunspot areas covering more than 130 years
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Modelling the Longitudinal Asymmetry in Sunspot Emergence: The Role of the Wilson Depression