Table 1.
Details of the BLAPs refered to in this study.
| ID | Period (min) | G (mag) | Parallax (mas) | d (pc) | (BP − RP) | MG | E(BP − RP) | MGo | (BP − RP)o |
|---|---|---|---|---|---|---|---|---|---|
| 1 | 28.26 | 17.503 ± 0.006 | 0.102 ± 0.091 | 5330 (3730–10480) | 0.358 ± 0.044 |
|
0.8 |
|
−0.44 ± 0.17 |
| 3 | 28.46 | 18.915 ± 0.010 | −0.117 ± 0.450 | 3480 (1920–9210) | 1.459 ± 0.093 |
|
1.5 |
|
−0.04 ± 0.31 |
| 4 | 22.36 | 18.469 ± 0.009 | 0.108 ± 0.229 | 3770 (2330–9310) | 1.500 ± 0.06 |
|
1.4 |
|
0.10 ± 0.29 |
| 6 | 38.02 | 18.174 ± 0.007 | 0.295 ± 0.302 | 2930 (1760–8450) | 1.160 ± 0.06 |
|
1.0 |
|
0.16 ± 0.21 |
| 9 | 31.94 | 15.574 ± 0.008 | 0.377 ± 0.047 | 2650 (2250–3470) | 0.626 ± 0.028 |
|
1.4 |
|
−0.77 ± 0.28 |
| 10 | 32.13 | 17.185 ± 0.009 | 0.147 ± 0.123 | 4370 (2970–9500) | 0.389 ± 0.055 |
|
1.4 |
|
−1.01 ± 0.29 |
| 11 | 34.87 | 17.250 ± 0.004 | −0.020 ± 0.185 | 4670 (2960–10310) | 0.231 ± 0.028 |
|
1.3 |
|
−1.07 ± 0.26 |
| 12 | 30.90 | 18.233 ± 0.012 | −1.252 ± 0.299 | 6170 (3860–12230) | 1.114 ± 0.067 |
|
1.4 |
|
−0.29 ± 0.29 |
| 13 | 39.33 | 18.931 ± 0.008 | 0.719 ± 0.409 | 1890 (1160–7430) | 1.505 ± 0.061 |
|
0.9 |
|
0.60 ± 0.19 |
| 14 | 33.62 | 16.804 ± 0.005 | 0.542 ± 0.143 | 1920 (1460–4380) | 0.014 ± 0.059 |
|
0.7 |
|
−0.69 ± 0.15 |
Notes. The columns show the BLAP ID based on the number convention of Pietrukowicz et al. (2017), from where the optical period is also taken; the mean Gaia G band mag; parallax and distance determined via a Bayesian approach and a scale parameter L = 1.35 kpc; the (BP − RP) (those in italics have been transformed from their (V − I) colour), the absolute G magnitude uncorrected for reddening, MG and extinction, E(BP − RP) (see text for details). The final columns, MGo and (BP − RP)o are the dereddened absolute G band magnitude and the dereddened (BP − RP) colour.
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