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Table 2.

Results of the time series analysis for all target stars.

PMF EPIC Campaign Frequency Amplitude SNR Type Upper Limit
0.03–0.5 0.5–2.0 2.0–25
[c/d] [Flux] [c/d] [c/d] [c/d]
2917-54556-0089 201381939 C102 0.30 0.15 0.09
2892-54552-0194 201434772 C102 0.50 0.25 0.18
0515-52051-0079 201634373 C01 0.18 0.12 0.12
3334-54927-0349 202066368 C00 0.61558(9) 0.0105(3) 12.3 GDOR
0.6594(5) 0.0094(3) 11.1
0.5808(1) 0.0080(3) 9.4
0.5475(7) 0.0048(3) 5.7
1.272(1) 0.0038(3) 4.9
3334-54927-0089 202066487 C00 0.18 0.18 0.15
2676-54179-0319 202066571 C00 0.5594(2) 0.00525(6) 38.0 ACV
0.2826(5) 0.00202(6) 14.4
0.3216(6) 0.00160(6) 11.4
0.842(1) 0.00092(6) 6.7
2676-54179-0272 202067375 C00 0.14 0.14 0.14
2676-54179-0317 202067392 C00 15.622(2) 0.00036(4) 7.7 DSCT
16.007(2) 0.00027(4) 5.6
14.317(3) 0.00026(4) 5.4
21.404(3) 0.00025(4) 4.9
15.150(3) 0.00021(4) 4.8
5293-55953-0322 211378898 C05, C18 15.3052(6) 0.023(2) 14.7 UGSU
2428-53801-0439 211477347 C16, C18 0.6093(1) 0.28(1) EA
2434-53826-0400 211617909 C05, C18 6.8339(2) 0.0125(4) 32.8 CV
13.6685(6) 0.0052(4) 16.8
20.5027(8) 0.0037(4) 14.4
2271-53726-0187 211823779 C05, C18 0.23 0.19 0.09
1924-53330-0016 212003762 C18 0.6476(4) 0.00194(6) 13.9 ROT
0.6227(5) 0.00143(6) 10.2
1.312(1) 0.00058(6) 4.7
1927-53321-0533 212108396 C05, C18 0.71 0.33 0.33
1929-53349-0356 212137838 C05 0.22416(4) 0.00554(3) 56.3 ROT
0.20862(9) 0.00279(3) 28.3
0.2414(3) 0.00091(3) 9.3
0.4569(3) 0.00073(3) 7.7
0.4373(4) 0.00069(3) 7.2
2315-53741-0286 212167054 C18 1.4501(4) 0.27(1) EA
2315-53741-0014 212168575 C05, C18 3.0421(2) 0.126(2) 26.4 RRc
6.085(1) 0.017(3) 7.4
9.127(2) 0.08(3) 5.8
2716-54628-0638 212682624 C06 1.4500(2) 0.00122(5) 21.0 ELL
3.309(1) 0.00025(5) 4.9
0696-52209-0410 220227479 C08 0.33 0.18 0.15
4550-55894-0172 220489294 C08 2.80 1.35 1.70
3779-55222-0306 228960916 C102 1.80 2.10 1.90
0381-51811-0200 246429212 C12 4.0908(2) 0.0039(1) 24.8 ELL
2.0460(6) 0.0014(1) 8.0
3834-56014-0026 248407521 C14 1.20 0.80 0.90
5357-55956-0482 248833732 C14 2.00 1.80 2.00
2304-53762-0140 251353301 C16 5.94660(5) 0.0881(8) 27.5 EW
2.9724(7) 0.0076(8) 4.7
8.9210(8) 0.0071(8) 5.5
17.840(1) 0.0052(8) 7.1
11.894(1) 0.0052(8) 6.1
23.787(1) 0.0046(8) 8.4

Notes. The errors in the final digits of the corresponding quantity are given in parentheses. The determined frequencies, amplitudes, and signal-to-noise ratios for the variable ones are listed in Cols. 4 to 6. For the eclipsing binaries EPIC 211477347 and 212167054, we list the mean depths of the primary minimum. The next column denotes the type of variability according to the abbreviations of the VSX (see notes below). The last three columns list the upper limits in different frequency domains. The absolute numbers depend on the time basis, apparent magnitude, and the observed sector. It should be noted that harmonics of frequencies were also detected. GDOR stands for γ Doradus star. ACV stands for α2 Canum Venaticorum variable. DSCT stands for the variable of the δ Scuti type. UGSU stands for U Geminorum-type variable, quite often called dwarf novae. EA stands for detached eclipsing binary. CV stands for cataclysmic variable. ROT stands for spotted star showing variability due to rotation. RRc stands for RR Lyrae type-c variable. ELL stands for rotating ellipsoidal variable. EW stands for W Ursae Majoris-type eclipsing binary.

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