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The frequency of low-mass exoplanets. II. The 'period valley'

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Figure

Table 2Planets from This Sample
Figure 1. Detectabilities obtained from Method 1 (solid contours) averaged overall 24 stars, for planets with eccentricities from 0.0 to 0.6
Figure 4. Same as Figure 2, but for HD 10700 (left) and HD 16417 (right).
Figure 5. Same as Figure 2, but for HD 20794 (left) and HD 23249 (right).
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