Table B.1.
Magnitude-dependent bias correction.
| F814W [mag] | M1 [M⊙] | N |  [%] |
 |
fcl [%] |
|---|---|---|---|---|---|
| 14.5−15.0 | 8.5−9.0 | 2 | 0 | 0.60 ± 0.35 | ... |
| 15.0−15.5 | 8.5−9.0 | 6 | 33 ± 19 | 0.61 ± 0.27 |  |
| 15.5−16.0 | 8.0−8.5 | 14 | 21 ± 11 | 0.53 ± 0.27 |  |
| 16.0−16.5 | 7.5−8.0 | 26 | 23 ± 8 | 0.51 ± 0.19 |  |
| 16.5−17.0 | 7.0−7.5 | 25 | 16 ± 7 | 0.41 ± 0.21 |  |
| 17.0−17.5 | 6.5−7.0 | 42 | 19 ± 6 | 0.44 ± 0.15 |  |
| 17.5−18.0 | 6.0−6.5 | 60 | 10 ± 4 | 0.45 ± 0.19 |  |
| 18.0−18.5 | 5.5−6.0 | 73 | 8 ± 3 | 0.30 ± 0.08 |  |
| 18.5−19.0 | 5.0−5.5 | 33 | 6 ± 4 | 0.26 ± 0.18 |  |
Notes. The magnitude bin is indicated in the first column, and the corresponding selected initial masses in the second column. In the third and fourth column we list the number of stars with measured RVs and the observed close binary fraction in the corresponding magnitude bin, respectively. The last two columns list the binary detection probability considering the combined SB1+SB2 bias and the bias-corrected close binary fraction.
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