Orbiting a binary - SPHERE characterisation of the HD 284149 system

M. Bonavita; V. D’Orazi; D. Mesa; C. Fontanive; S. Desidera; S. Messina; S. Daemgen; R. Gratton; A. Vigan; M. Bonnefoy; A. Zurlo; J. Antichi; H. Avenhaus; A. Baruffolo; J. L. Baudino; J. L. Beuzit; A. Boccaletti; P. Bruno; T. Buey; M. Carbillet; E. Cascone; G. Chauvin; R. U. Claudi; V. De Caprio; D. Fantinel; G. Farisato; M. Feldt; R. Galicher; E. Giro; C. Gry; J. Hagelberg; S. Incorvaia; M. Janson; M. Jaquet; A. M. Lagrange; M. Langlois; J. Lannier; H. Le Coroller; L. Lessio; R. Ligi; A. L. Maire; M. Meyer; F. Menard; C. Perrot; S. Peretti; C. Petit; J. Ramos; A. Roux; B. Salasnich; G. Salter; M. Samland; S. Scuderi; J. Schlieder; M. Surez; M. Turatto; L. Weber

doi:10.1051/0004-6361/201731003

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Volume 608 (December 2017)

A&A, 608 (2017) A106

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Fig. 6

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Left panel: pooled variance profile of HD 284149 computed on the SuperWASP V-mag time series. Right Panel: long-term V-band magnitude time series of HD 284149.

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