Extrasolar planets and brown dwarfs around AF-type stars - X. The SOPHIE sample: combining the SOPHIE and HARPS surveys to compute the close giant planet mass-period distribution around AF-type stars

S. Borgniet; A.-M. Lagrange; N. Meunier; F. Galland; L. Arnold; N. Astudillo-Defru; J.-L. Beuzit; I. Boisse; X. Bonfils; F. Bouchy; K. Debondt; M. Deleuil; X. Delfosse; M. Desort; R. F. Díaz; A. Eggenberger; D. Ehrenreich; T. Forveille; G. Hébrard; B. Loeillet; C. Lovis; G. Montagnier; C. Moutou; F. Pepe; C. Perrier; F. Pont; D. Queloz; A. Santerne; N. C. Santos; D. Ségransan; R. da Silva; J. P. Sivan; S. Udry; A. Vidal-Madjar

doi:10.1051/0004-6361/201833431

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Volume 621 (January 2019)

A&A, 621 (2019) A87

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Fig. 10

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Properties of our combined sample (SOPHIE +HARPS). Top left panel: position of our targets in an H–R diagram. Blue diamonds: SOPHIE targets; orange crosses: HARPS targets. The Sun is displayed (red star) for comparison. Top right panel: stellar mass histogram of our combined sample. Blue: SOPHIE targets; orange: HARPS targets. Bottom left panel: spectrum number per target. Bottom right panel: timebase histogram.

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