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Table A.1

Radial velocities derived from the G-band for SDSS J0929+0238.

Date UT MJD Vrad BARYCOR
(JD–2 400 000.5) [km s-1] [km s-1]

2015-01-25 07:33:37.533 57 047.315017751 390.56 9.528105
2015-02-19 01:48:44.237 57 072.075512012 404.48/376.90 − 2.633427
2015-11-20 07:03:07.093 57 346.293832105 392.20 29.748689
2016-01-15 04:42:58.393 57 402.196509185 391.35 14.807685
2016-01-15 05:41:22.486 57 402.23706582 391.23 14.688431
2016-01-15 06:32:46.452 57 402.27275987 391.72 14.578024
2016-01-15 03:51:40.927 57 402.16089037 391.74 14.902034
2016-01-15 07:25:37.326 57 402.309459796 391.90 14.464483
2016-02-14 03:06:44.969 57 432.129687148 398.95/384.56 − 0.069693
2016-02-14 02:15:09.096 57 432.09385528 399.66/385.27 0.032276
2016-02-15 00:47:02.669 57 433.032669787 407.97/382.79/362.41 − 0.34363
2016-03-05 00:50:42.637 57 452.035215711 398.40/383.71 − 9.922114
2016-03-05 01:43:58.919 57 452.072209719 398.89/385.70 − 10.024746
2016-03-06 00:56:38.000 57 453.03944384 388.91/374.22 − 10.416031
2016-03-06 01:50:02.879 57 453.076422215 388.61/373.62 − 10.520604
2016-03-06 02:43:48.203 57 453.113752352 387.71/373.02 − 10.63447

Notes. When multiple peaks are detected in the CCF, the velocities reported in Col. 4 are ordered by the largest to the smallest. We have not attempted to associate each velocity to one of the stellar components in the system. The stars have very similar luminosities, therefore it is not easy to distinguish between them. As such, to avoid giving misleading information this will be addressed when further data is secured. The uncertainty is of the order of 1 km s-1 for the single-peaked CCFs. Conservatively, we think it can be larger (within 2 km s-1) due to the uncertainty in the fitting of multiple peaks.

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