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Cited article:
A. I. Shapiro, S. K. Solanki, N. A. Krivova, W. K. Schmutz, W. T. Ball, R. Knaack, E. V. Rozanov, Y. C. Unruh
A&A, 569 (2014) A38
Published online: 2014-09-16
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Activity time series of old stars from late F to early K
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Power spectra of solar brightness variations at various inclinations
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Solar-cycle irradiance variations over the last four billion years
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Solar-type Stars Observed by LAMOST and Kepler
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Photometric Variability as a Proxy for Magnetic Activity and Its Dependence on Metallicity
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Predictions of Astrometric Jitter for Sun-like Stars. I. The Model and Its Application to the Sun as Seen from the Ecliptic
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Where Have All the Solar-like Stars Gone? Rotation Period Detectability at Various Inclinations and Metallicities
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Indications for very high metallicity and absence of methane in the eccentric exo-Saturn WASP-117b
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Scrutinising the relationship between plage areas and sunspot areas and numbers
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How faculae and network relate to sunspots, and the implications for solar and stellar brightness variations
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The relationship between bipolar magnetic regions and their sunspots
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Faculae Cancel out on the Surfaces of Active Suns
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Predictions of Astrometric Jitter for Sun-like Stars. III. Fast Rotators
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Unsigned Magnetic Flux as a Proxy for Radial-velocity Variations in Sun-like Stars
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Starspots, chromospheric emission lines, and flares of zero-age main-sequence stars
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