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

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Fig. 16

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Constraints on companion occurrence rates from our combined SOPHIE + HARPS survey. From top to bottom panels: brown dwarf companions (13–80 M_Jup), Jupiter-mass companions (1–13 M_Jup), Saturn-masscompanions (0.3–1 M_Jup). From left to right on each row: period ranges of 1–10, 10–100, and 100–1000 days. Cyan: stellar mass ≤1.5 M_⊙ subsample (with 1σ error bars in blue). Orange: stellar mass >1.5 M_⊙ subsample (with 1σ error bars in red). Actual occurrence rates are displayed in full colour (n_det ≥ 1) and upperlimits (n_det = 0) are displayed in hatch.

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