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Table 3:

Properties of the short period stars.
ID $\alpha$ [hms] $\delta$ [dms] $d~[\hbox{$^{\prime\prime}$ }]$ f [d-1] SNR
V73 13:13:03.1 18:09:26.1 119.9 14.26581 10.2
V74 13:12:49.7 18:07:26.3 181.9 22.03949 13.7
V75 13:13:09.4 18:09:39.5 203.9 22.60022 11.8
V76 13:13:05.0 18:08:35.3 168.4 24.10224 10.4
V77* 13:13:20.8 18:15:34.9 488.3 13.00995 23.0
V78* 13:12:49.8 18:08:56.0 106.9 22.25488 12.7
V79* 13:12:46.6 18:11:36.9 150.6 21.59184 9.7
V80* 13:12:57.4 18:10:13.8 31.3 14.83029 14.2
V81* 13:13:02.7 18:06:29.4 244.5 14.01180 9.5
V82* 13:12:56.5 18:13:10.0 181.1 45.33103 8.4
V83* 13:12:50.1 18:07:42.9 164.5 8.01907 8.2

Notes: new discoveries are marked with asterisks. The signal-to-noise ratio (SNR) was calculated in the [0,50] d-1 frequency range. See Table 1 for other notations.


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