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Table 1.

Extracted frequencies of HD 170580 with amplitude above five times the local noise level.

# f (d−1) A (ppm) S/N Notes
f1 3.3373(4) 148(17) 23.8 quintuplet
f2 3.2371(5) 103(16) 11.4 triplet
f3 1.7957(6) 82(15) 11.4 triplet, in HARPS spectra
f4 3.3509(6) 87(15) 11.4 quintuplet
f5 1.8622(6) 72(14) 11.4 triplet
f6 3.3233(7) 71(15) 11.4 quintuplet
f7 1.8364(7) 61(13) 11.9 triplet
f8 1.7221(8) 53(13) 12.2 triplet
f9 3.3066(9) 54(14) 11.6 quintuplet
f10 1.9691(9) 49(14) 12.4
f11 1.5426(7) 48(10) 11.2 f1 − f3
f12 3.2237(10) 46(14) 11.9 triplet
f13 1.5559(6) 42(8) 8.5 f4 − f3
f14 3.4432(11) 39(14) 12.2
f15 1.6950(7) 36(8) 8.6 triplet
f16 1.8095(6) 46(8) 8.8
f17 1.8008(6) 41(8) 8.9 unresolved
f18 3.2505(12) 37(13) 12.5 triplet, f13 + f15
f19 1.7083(8) 31(8) 9.1 triplet
f20 1.5151(8) 33(8) 9.3 f2 − f8
f21 1.4822(7) 28(6) 9.0 f6 − f7
f22 3.3895(9) 29(8) 9.1 f7 + f13?
f23 3.6568(9) 29(8) 9.1 triplet, f3 + f5
f24 1.8495(10) 24(8) 9.4 triplet
f25 1.5285(8) 24(6) 7.4 f1 − f16
f26 1.7849(9) 22(6) 7.2 triplet
f27 3.7348(11) 23(8) 9.3
f28 3.2902(13) 20(8) 9.3 f16 + f21?
f29 3.5936(13) 20(8) 9.3 f3 + f17
f30 3.8053(12) 22(8) 9.3 f7 + f10
f31 3.6715(13) 20(8) 9.3 triplet, f5 + f16?
f32 2.2010(9) 21(6) 7.5
f33 3.4567(12) 21(8) 9.3 f10 + f21?
f34 3.4040(12) 21(8) 9.3 f15 + f19?, f5 + f11?
f35 1.5694(6) 18(3) 6.8 f4 − f19
f36 1.8880(8) 23(6) 7.5 f27 − f24?
f37 1.7510(10) 19(6) 7.6 f14 − f15? f2 − f21?
f38 8.4401(28) 19(16) 11.3 f3 + 2f6
f39 3.3641(11) 18(6) 7.4 quintuplet
f40 1.7727(7) 16(3) 6.8 triplet
f41 2.0069(6) 17(3) 6.9 satellite
f42 3.1905(13) 14(6) 7.7 f19 + f21?
f43 3.6433(12) 15(6) 7.7 triplet, f3 + f24?

fS1 2.6700 in HERMES spectra
alias of f31

Notes. The formal errors from a NLLS fit were corrected for the correlated nature of the data following Schwarzenberg-Czerny (2003) and are indicated in brackets at the level of the last digits. The significance (in terms of S/N) was computed over an interval of 2 d−1 centred on the pre-whitened frequency. The frequencies in italic are omitted in the interpretation; a discussion of the notes can be found in the text. The last row lists the dominant frequency found in the HERMES spectroscopy, while f3 was recovered in the HARPS spectra.

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