Table B.5
Estimated p-values from the Anderson–Darling (AD) tests for the distributions of Teff and [Fe/H] between all the Kepler targets, all the KOIs, the giant-planet hosts, and false-positive hosts.
| Stellar effective temperature | |||
|
|
|||
| All targets | All KOIs | Giant planets | |
|
|
|||
| All KOIs | 2.4 ×10-5 | – | – |
| Giant planets | 7.6 ×10-4 | 1.5 ×10-3 | – |
| False positives | 0.088 | 0.061 | 0.062 |
|
|
|||
| Stellar iron abundance | |||
|
|
|||
| All targets | All KOIs | Giant planets | |
|
|
|||
| All KOIs | 9.7 ×10-6 | – | – |
| Giant planets | 1.4 ×10-5 | 4.6 ×10-5 | – |
| False positives | 0.61 | 0.50 | 2.2 ×10-4 |
Notes. Note that for speeding up the computation of the AD test, we took only one Kepler target over 10. We tested that the conclusions are unchanged using different (but large enough) sub-sample of the Kepler targets.
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