Table A.1.
Synthetic samples of dark companion, semidetached, and contact binary light curves.
| Sample | σWN (mag) | σCN | lCN |
|---|---|---|---|
| W0C0 | – | – | – |
| W0C1L25 | – | 0.01 | 0.25 |
| W0C1L50 | – | 0.01 | 0.50 |
| W0C1L100 | – | 0.01 | 1.00 |
| W0C5L25 | – | 0.05 | 0.25 |
| W0C5L50 | – | 0.05 | 0.50 |
| W0C5L100 | – | 0.05 | 1.00 |
| W0C10L25 | – | 0.10 | 0.25 |
| W0C10L50 | – | 0.10 | 0.50 |
| W0C10L100 | – | 0.10 | 1.00 |
| W1C0 | 10−4 | – | – |
| W1C1L25 | 10−4 | 0.01 | 0.25 |
| W1C1L50 | 10−4 | 0.01 | 0.50 |
| W1C1L100 | 10−4 | 0.01 | 1.00 |
| W1C5L25 | 10−4 | 0.05 | 0.25 |
| W1C5L50 | 10−4 | 0.05 | 0.50 |
| W1C5L100 | 10−4 | 0.05 | 1.00 |
| W1C10L25 | 10−4 | 0.10 | 0.25 |
| W1C10L50 | 10−4 | 0.10 | 0.50 |
| W1C10L100 | 10−4 | 0.10 | 1.00 |
| W10C0 | 10−3 | – | – |
| W10C1L25 | 10−3 | 0.01 | 0.25 |
| W10C1L50 | 10−3 | 0.01 | 0.50 |
| W10C1L100 | 10−3 | 0.01 | 1.00 |
| W10C5L25 | 10−3 | 0.05 | 0.25 |
| W10C5L50 | 10−3 | 0.05 | 0.50 |
| W10C5L100 | 10−3 | 0.05 | 1.00 |
| W10C10L25 | 10−3 | 0.10 | 0.25 |
| W10C10L50 | 10−3 | 0.10 | 0.50 |
| W10C10L100 | 10−3 | 0.10 | 1.00 |
| W100C0 | 10−2 | – | – |
| W100C1L25 | 10−2 | 0.01 | 0.25 |
| W100C1L50 | 10−2 | 0.01 | 0.50 |
| W100C1L100 | 10−2 | 0.01 | 1.00 |
| W100C5L25 | 10−2 | 0.05 | 0.25 |
| W100C5L50 | 10−2 | 0.05 | 0.50 |
| W100C5L100 | 10−2 | 0.05 | 1.00 |
| W100C10L25 | 10−2 | 0.10 | 0.25 |
| W100C10L50 | 10−2 | 0.10 | 0.50 |
| W100C10L100 | 10−2 | 0.10 | 1.00 |
Notes. Each sample contains a total of 42 700 light curves (11 220 dark companion, 18 460 semidetached, and 13 020 contact binaries) generated with a different combination of uncorrelated noise standard deviation σWN, correlated noise standard deviation σCN (proportional to the unperturbed light curve amplitude), and correlation length scale lCN (in units of the orbital period).
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