Table 8.
Information about the eclipsing binary candidates identified in the present study.
| ID | HSP | J | H | K | ptpJ | ptpH | ptpK | Type | Per | Perrot |
|---|---|---|---|---|---|---|---|---|---|---|
| (CygOB2-) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (d) | (d) | ||
| 000644 | 21 | 13.68 | 13.14 | 12.93 | 0.08 | 0.08 | 0.08 | 3 | 2.89 (1.44/3.21) | – |
| 010997 | 11.54 | 10.88 | 10.48 | 0.10 | 0.11 | 0.10 | 3 | – | – | |
| 041491 | 14.31 | 13.23 | 12.73 | 0.16 | 0.16 | 0.17 | 3 | 1.58/3.77 | 7.39 | |
| 041510 | 11.80 | 11.10 | 10.70 | 0.28 | 0.23 | 0.28 | 3 | 4.69 | – | |
| 041524 | 16.29 | 15.03 | 14.45 | 0.17 | 0.16 | 0.19 | 3 | – | – | |
| 041588 | 10.45 | 9.97 | 9.66 | 0.25 | 0.23 | 0.21 | 3 | 1.11 | – | |
| 072104 | 58 | 14.59 | 13.95 | 13.65 | 0.33 | 0.30 | 0.31 | 3 | 0.83 | – |
| 072174 | 106 | 15.28 | 14.22 | 13.74 | 0.21 | 0.23 | 0.25 | 3 | 7.30 | – |
| 103439 | 11.64 | 11.24 | 10.98 | 0.14 | 0.18 | 0.15 | 3 | – | – | |
| 103616 | 15.52 | 14.44 | 13.93 | 0.26 | 0.23 | 0.22 | 3 | 1.14 | – | |
| 114036 | 15.54 | 14.28 | 13.67 | 0.16 | 0.14 | 0.15 | 3 | 0.90 | – | |
| 114133 | 16.18 | 15.06 | 14.54 | 0.33 | 0.27 | 0.30 | 3 | 1.97/3.95 | ||
| 124487 | 14.51 | 13.40 | 12.88 | 0.22 | 0.21 | 0.20 | 3 | 4.77 | 1.12 | |
| 134771 | 12.80 | 12.04 | 11.61 | 0.06 | 0.06 | 0.07 | 3 | – | – | |
| 114152 | 92 | 15.34 | 14.54 | 14.12 | 0.43 | 0.40 | 0.40 | 1 | 0.42 (3.36) |
Notes. The table shows the internal ID for each star. HSP indicates their ID in HSP11, J, H, and K indicates their median magnitudes in each band, and the ptp fields show their peak to peak amplitude in each band. Type gives their morphological classification: 1 if periodic and 3 if occultation. Per gives the period detected for the eclipse, and Perrot gives the rotational period, when measured.
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