Table A.2.
Photometry for stars observed spectroscopically in this work.
| Star | Va | (B − V)a | Jb | Hb |  |
Gc | (GBP − GRP)c | E(GBP − GRP)c |  |
|---|---|---|---|---|---|---|---|---|---|
| Members | |||||||||
| 0305 | 12.359 | 0.654 | 11.178 | 10.854 | 10.813 | 12.231 | 0.836 | 0.000 | 0.002 |
| 2451 | 7.318* | 0.121* | 7.312 | 7.353 | 7.351 | 7.358 | −0.023 | 0.041 | 0.076 |
| 3061 | 11.256 | 0.466 | 10.329 | 10.141 | 10.097 | 11.141 | 0.620 | 0.001 | 0.001 |
| 3288 | 12.698 | 0.751 | 11.474 | 11.144 | 11.075 | 12.602 | 0.889 | 0.023 | 0.042 |
| 3311 | 10.168 | 0.296 | 9.587 | 9.524 | 9.468 | 10.110 | 0.396 | 0.032 | 0.060 |
| 3781 | 6.961* | 0.139* | 6.826 | 6.846 | 6.890 | 6.831 | −0.036 | 0.051 | 0.096 |
| 3814 | 7.630* | 0.057* | 7.663 | 7.608 | 7.668 | 7.663 | −0.004 | 0.040 | 0.075 |
| 4265 | 8.228 | 0.029 | 8.104 | 8.084 | 8.107 | 8.252 | 0.056 | 0.132 | 0.247 |
| 4322 | 12.403 | 0.646 | 11.193 | 10.866 | 10.826 | 12.249 | 0.832 | 0.001 | 0.001 |
| 4438 | 11.447 | 0.535 | 10.503 | 10.288 | 10.223 | 11.329 | 0.651 | 0.003 | 0.005 |
| 4673 | 9.008 | 0.082 | 8.874 | 8.898 | 8.875 | 9.035 | 0.088 | 0.110 | 0.206 |
| 5045 | 6.691* | 0.195* | 6.697 | 6.778 | 6.728 | 6.840 | 0.012 | 0.048 | 0.091 |
| 5609 | 10.460 | 0.308 | 9.713 | 9.567 | 9.521 | 10.343 | 0.477 | 0.016 | 0.029 |
| 5729 | 9.356 | 0.176 | 9.041 | 8.997 | 8.993 | 9.369 | 0.204 | 0.032 | 0.060 |
| 6791 | 9.565 | 0.286 | 9.267 | 9.142 | 9.181 | 9.562 | 0.220 | ... | ... |
| 7140 | 9.392 | 0.355 | 9.150 | 9.132 | 9.072 | 9.405 | 0.179 | 0.022 | 0.041 |
| ucac | 12.649 | 0.633 | 11.403 | 11.098 | 11.010 | 12.480 | 0.847 | 0.058 | 0.108 |
| Non-members | |||||||||
| 3004 | 10.428 | 0.354 | 9.927 | 9.793 | 9.746 | 10.526 | 0.466 | 0.024 | 0.045 |
| 3423 | 10.932 | 0.508 | 10.013 | 9.673 | 9.674 | 10.813 | 0.668 | 0.001 | 0.003 |
| 4294 | 6.813 | 0.207 | 6.478 | 6.470 | 6.513 | 6.573 | 0.018 | ... | ... |
Notes. a From the APASS catalogue (Henden et al. 2016). b From the 2MASS catalogue (Skrutskie et al. 2006). c From the Gaia-DR3 catalogue (Gaia Collaboration 2023). * Scaled from the V and (B − V) values of Kharchenko & Roeser (2009) and the relation proposed in the present work.
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