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Table A.2.

Periods, mean magnitudes, and amplitudes as derived from various light curves for all periodically variable white dwarfs showing only the He II line problem.

Name Band Data points Magnitude P Amplitude Comment
[mag] [d] [mag]
J0821+1739 CSS 275 19.14 0.384835 ± 0.000084 0.13 DOZ UHE:
K2 2478 19.32 0.384878 ± 0.000006
J1029+2540 CSS 470 17.11 0.282933 ± 0.000016 0.04 DO UHE:
ZTF-g 130 16.85 0.282932 ± 0.000007 0.05
ZTF-r 144 17.39 0.282926 ± 0.000011 0.04
HE 1314+0018 TESS 13449 0.524170 ± 0.001505 DOZ
J1512+0651 ZTF-r 119 17.56 0.226022 ± 0.000010 0.06
HS 1517+7403 ZTF-g 259 16.42 1.091158 ± 0.000057 0.05 DOZ
ZTF-r 237 16.97 1.091142 ± 0.000011 0.04 DO
TESS 94063 1.091338 ± 0.000278 DOZ
J1553+4832 ZTF-g 1203 18.42 2.928482 ± 0.000462 0.05 DO
ZTF-r 1261 18.97 2.928408 ± 0.000990 0.04

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