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Table 3
Gradients of corrected exoplanet frequency for stars up to 16th magnitude in Cartesian coordinates (x, y, z).
| Sp. type | kx, pc−1 | Error | ky, pc−1 | Error | kz, pc−1 | Error |
|---|---|---|---|---|---|---|
| Rplanet ≥ 0.75 REarth | ||||||
| F | 6.0 × 10−4 | 5.1 × 10−4 | − 5.5 × 10−4 | 1.9 × 10−4 | 7.7 × 10−4 | 5.7 × 10−4 |
| G | 5.7 × 10−4 | 9.8 × 10−4 | − 1.0 × 10−4 | 3.7 × 10−4 | 1.1 × 10−3 | 1.0 × 10−3 |
| K | Number of objects is too low for statistics | |||||
| 0.75 REarth ≤ Rplanet ≤ 1.75 REarth | ||||||
| F | 2.9 × 10−3 | 3.3 × 10−3 | − 3.0 × 10−3 | 1.1 × 10−3 | 4.5 × 10−3 | 3.1 × 10−3 |
| G | 6.0 × 10−4 | 2.1 × 10−3 | − 2.4 × 10−4 | 8.0 × 10−4 | 3.5 × 10−3 | 2.1 × 10−3 |
| K | Number of objects is too low for statistics | |||||
| 1.75 REarth ≤ Rplanet < 3.0 REarth | ||||||
| F | 4.4 × 10−5 | 1.5 × 10−3 | − 1.4 × 10−3 | 5.8 × 10−4 | 3.6 × 10−3 | 1.8 × 10−3 |
| G | 2.2 × 10−3 | 1.7 × 10−3 | − 4.3 × 10−4 | 6.3 × 10−4 | 2.7 × 10−4 | 1.7 × 10−3 |
| K | Number of objects is too low for statistics | |||||
| Rplanet ≥ 3.0 REarth | ||||||
| F | 3.2 × 10−4 | 3.7 × 10−4 | 1.1 × 10−5 | 1.3 × 10−4 | − 2.9 × 10−4 | 3.7 × 10−4 |
| G | − 4.0 × 10−4 | 7.9 × 10−4 | 4.1 × 10−4 | 3.0 × 10−4 | − 3.1 × 10−4 | 8.1 × 10−4 |
| K | Number of objects is too low for statistics | |||||
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