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Table 2.

Parameters of detected TEOs.

Star Frequency Amplitude n Δn(a)
f (d−1) (ppt) (10−3)
QX Car 1.1162(9) 0.156(14) 5 −0.3(9)
1.5630(7) 0.221(14) 7 −0.2(7)
2.2295(10) 0.131(14) 10 −3.6(10)*
2.6784(10) 0.137(14) 12 −1.3(10)
p Vel A 0.49897(22) 0.1346(23) 5 +94.7(23)*
0.7909(6) 0.0458(22) 8 +76(6)*
1.0798(4) 0.0562(20) 11 +25(4)*
1.7553(10) 0.0235(20) 18 −77(10)*
θ1 Cru 0.16530(18) 0.1184(19) 4 +1.92(18)*
0.28623(16) 0.1999(25) 7 +0.32(16)
0.3667(3) 0.0836(22) 9 −0.1(3)
0.40722(16) 0.1536(21) 10 −1.23(16)*
0.53127(19) 0.1255(22) 13 +0.29(20)
0.56975(23) 0.1029(23) 14 −2.08(23)*
0.6117(4) 0.0593(22) 15 −1.0(4)
ζ1 UMa 0.14628(4) 0.0394(10) 3 +0.21(4)*
0.24339(13) 0.0140(10) 5 −0.06(13)
0.29193(10) 0.0181(11) 6 −0.20(10)
0.38923(15) 0.0111(10) 8 −0.28(15)
0.48701(16) 0.0101(10) 10 +0.12(16)
0.82794(16) 0.0103(10) 17 +0.23(16)
1.31475(26) 0.0063(10) 27 +0.15(26)
1.75388(21) 0.0078(9) 36 +1.07(21)*
V1294 Sco 1.2529(16) 1.14(9) 7 +3.9(16)
HD 158013 0.85199(4) 0.0468(8) 7 −0.02(4)
1.095404(7) 0.2078(8) 9 −0.033(7)*
2.19074(6) 0.0229(8) 18 −0.14(6)
14 Peg 1.5066(18) 0.040(4) 8 −1.5(18)
3.2062(18) 0.041(4) 17 +1.5(18)

Notes.

(a)

Δn = f/forb − n, where f is the detected frequency (second column). Frequencies with |Δn| exceeding 3σΔn are marked with an asterisk in the fifth column.

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