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Table A.2

Fourier parameters of single-mode Cepheids (excerpt)

Name poly NDOF χ2 upsi;γ [km s−1] Ap2p [km s−1] A1 [km s−1] ϕ1 [rad] R21 ϕ21 [rad] R31 ϕ31 [rad] R41 ϕ41 [rad] R51 ϕ51 [rad]
AA Gem - 42 137.5 19.608 39.880 17.355 -1.317 0.0511 0.72 0.1444 5.81 0.0759 3.94 0.0170 1.54
AB Cam - 14 999.7 -43.980 47.204 16.814 -1.524 0.4957 4.71 0.2981 3.37 0.1551 1.93 0.0810 0.38
AC Mon - 47 1420.7 60.494 38.814 14.542 -1.355 0.5818 5.32 0.1397 3.95 0.1185 2.80 0.0223 1.83
AD Pup 4 93 2359.3 72.908 52.429 22.918 -1.337 0.0936 4.77 0.1075 5.82 0.1000 4.16 0.0449 2.67
AH Vel 1 57 17218.1 26.815 16.852 8.467 -1.544 0.1301 5.04 0.0436 3.23 0.0085 1.69 0.0181 5.89
AK Cep - 6 143.5 -53.950 36.077 14.119 -1.517 0.4548 4.72 0.2124 3.60 0.0810 2.18 0.0410 0.45
AN Aur - 24 205.6 4.094 33.243 13.759 -1.230 0.5051 5.88 0.1796 4.14 0.0890 3.70 0.0573 1.74
...

Notes. Fourier parameters were determined as explained in Sect. 3.1, and Fourier ratios are computed as described in Sect. 3.2. Stars exhibiting long-term trends of υγ were modeled using polynomials, and column ‘poly’ states its degree. NDOF = Nobs − 1 − Nmodel states the number of degrees of freedom of the fit, i.e., with Nmodel = 1 + 2 • NFS + poly the number of model parameters. χ2 has the usual meaning; high values of χ2 indicate unmodeled signals, cf. Sect. 4.3. υγ is the constant term of the fitted Fourier series, cf. Eqs. 2 and 3. Note that υγ does not correspond to the barycentric velocity for SB1 Cepheids. Ap2p is the peak-to-peak RV curve amplitude determined from the Fourier fit. A1 and ϕ1 are the semi-amplitude and Fourier phase of the first harmonic, respectively. Ri1 and Φil are the amplitudes and phase ratios of the i–th harmonic relative to the first (Simon & Lee 1981). Uncertainties for all parameters are provided in the data files as explained in App. C. The full table is available via the CDS.

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