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Table 4:

Properties of the long period variables.

ID
$\alpha$ [hms] $\delta$ [dms] $d~[\hbox{$^{\prime\prime}$ }]$ P [d] SNR V V-I
V84 13:12:36.2 18:07:32.3 306.6 22.4 15.5 14.766 1.175
V85 13:12:50.7 18:10:39.7 69.7 19.8 19.2 13.962 1.357
V86 13:12:52.7 18:10:28.0 39.4 22.2 12.9 $\sim$14.2 ...

Notes: for variable V86, only instrumental V magnitude average is shown because the star was saturated in the I band. The signal-to-noise ratio (SNR) was calculated in the [0,20] d-1 frequency range.


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