19 Oct 2010: Simpson et al. (2010) infer the orbital inclination 44 deg. from the parent star rotation, deriving a planet mass 1.5+2.5-0.5MJ; but the coplanarity of stellar equator with planet orbits is generally not demonstrated. 20 oct. 2002: The hypothetical planet epsilon Eridani c is suspected from the dust ring morphology (Quillen & Thorndike 2002) 2001:Marcy et al. claim that " The Doppler behavior of magnetically active stars remains poorly explored, because so few stars are as active as Epsilon Eridani. Thus, Campbell's interpretation of a planet remains controversial."
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BAAS
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The Geneva-Copenhagen survey of the Solar neighbourhood.
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BAAS
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Modeling the Infrared Emission from the epsilon Eridani Disk.
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Photospheric Abundances of Volatile and Refractory Elements in
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The Actual Mass of the Object Orbiting Epsilon Eridani.
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A dust ring around Epsilon Eridani : analogue to the young Solar System
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Correlation of the Radial Velocity of Epsilon Eridani with Its Magnetic
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BAAS
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A search for Jupiter-mass companions to nearby stars
WALKER G. A. H., WALKER A. R., IRWIN A. W., LARSON A.
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Epsilon Eridani's Planetary Companion and Circumstellar Dust.