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Table A.3

Same as in the Table 3 but the gradients of exoplanet frequency are not corrected for the observational biases.

Sp. type kx, pc−1 Error ky, pc−1 Error kz, pc−1 Error
Rplanet ≥ 0.75 REarth

F 1.09 × 10−5 2.0 × 10−5 −2.57 × 10−5 7.3 × 10−6 1.08 × 10−5 2.1 × 10−5
G − 3.82 × 10−6 7.4 × 10−5 − 2.57 × 10−5 2.7 × 10−5 3.50 × 10−5 7.5 × 10−5
K 3.08 × 10−4 1.6 × 10−3 − 3.66 × 10−4 5.7 × 10−4 − 7.29 × 10−5 1.6 × 10−3

0.75 REarthRplanet ≤ 1.75 REarth

F 9.24 × 10−6 1.5 × 10−5 −1.73 × 10−5 5.4 × 10−6 1.17 × 10−5 1.5 × 10−5
G 3.73 × 10−6 5.2 × 10−5 − 2.32 × 10−5 1.9 × 10−5 4.13 × 10−5 5.3 × 10−5
K 2.08 × 10−4 1.5 × 10−3 − 3.80 × 10−4 5.5 × 10−4 7.78 × 10−5 1.5 × 10−3

1.75 REarthRplanet < 3.0 REarth

F 7.42 × 10−7 1.0 × 10−5 − 7.82 × 10−6 3.7 × 10−6 4.82 × 10−6 1.0 × 10−5
G 1.43 × 10−5 4.2 × 10−5 − 1.12 × 10−5 1.5 × 10−5 − 1.35 × 10−6 4.3 × 10−5

K 24 planets - too few for statistics

Rplanet ≥ 3.0 REarth

F 9.34 × 10−7 8.7 × 10−6 − 5.84 × 10−7 3.1 × 10−6 − 5.68 × 10−6 8.8 × 10−6
G − 2.18 × 10−5 2.5 × 10−5 8.74 × 10−6 9.1 × 10−6 − 4.91 × 10−6 2.6 × 10−5

K 6 planets - too few for statistics

Notes. Statistically significant gradients (>3σ) are highlighted in boldface.

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