MAGNETIC ACTIVITY CYCLES IN THE EXOPLANET HOST STAR ϵ ERIDANI

ERRATUM: “CONFIRMING FUNDAMENTAL PROPERTIES OF THE EXOPLANET HOST STAR ϵ ERIDANI USING THE NAVY OPTICAL INTERFEROMETER” (2012, ApJ, 744, 138B)

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THE HARPS-TERRA PROJECT. I. DESCRIPTION OF THE ALGORITHMS, PERFORMANCE, AND NEW MEASUREMENTS ON A FEW REMARKABLE STARS OBSERVED BY HARPS

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MAGNETIC CYCLES IN A CONVECTIVE DYNAMO SIMULATION OF A YOUNG SOLAR-TYPE STAR

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EVIDENCE FOR THE IMPACT OF STELLAR ACTIVITY ON THE DETECTABILITY OF SOLAR-LIKE OSCILLATIONS OBSERVED BYKEPLER

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CHROMOSPHERIC ACTIVITY AND JITTER MEASUREMENTS FOR 2630 STARS ON THE CALIFORNIA PLANET SEARCH

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A SEISMIC SIGNATURE OF A SECOND DYNAMO?

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DISCOVERY OF A 1.6 YEAR MAGNETIC ACTIVITY CYCLE IN THE EXOPLANET HOST STAR ι HOROLOGII

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Parent stars of extrasolar planets - X. Lithium abundances andvsin irevisited

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The Chemical Composition of the Sun

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Exploring thePcycvs.Protrelation with flux transport dynamo models of solar-like stars

(2009) L. Jouve et al.   ASTRONOMY & ASTROPHYSICS

Mg II h+k emission lines as stellar activity indicators of main sequence F-K stars

(2008) A. P. Buccino et al.   ASTRONOMY & ASTROPHYSICS

Lithium depletion and the rotational history of exoplanet host stars

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Rapidly Rotating Suns and Active Nests of Convection

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