Notes. G lists the intensity-averaged Gaia DR3 G–band magnitude (int_average_g) from table gaiadr3.vari_cepheids unless preceded by a †, in which case phot_g_mean_mag from table gaiadr3.source was adopted because these stars were not included in the SOS processing (Ripepi et al. 2023). This was the case for ASAS J082710-3825.9, BB Gem, BB Sgr, FM Aql, RT Aur, SZ Aql, T Mon, TT Aql, TZ Mon, U Sgr, β Dor, and ζ Gem. Analogously, G_Bp − G_Rp is the intensity averaged Gaia DR3 color obtained from gaiadr3.vari_cepheids, or from gaiadr3.gaia_source. Column ‘Mode’ lists pulsation mode assignments according to gaiadr3.vari_cepheids. Column ‘SB1’ is ‘T’ for ‘True’ if the star exhibits clear signs of orbital motion either over the VELOCE baseline or in the template fitting analysis including literature data, ‘U’ for ‘Unsure’ if the signal is tentative, and ‘F’ for ‘False’ otherwise. Note that very long-period binaries may thus be labeled as ‘F’. Columns N_obs and N_FS list the number of VELOCE observations and the number of Fourier harmonics used to represent the pulsational RV variability. Columns P and σ_P specify the pulsation period and its total uncertainty. Analogously for the epoch E and σ_E, which is defined so that pulsation phase phi = 0 at υγ on the descending RV branch (minimum radius), cf. Sect. 3.1. Stars for which no models were fitted for various reasons are listed separately as labeled. Time-series RV measurements are published as part of this data release, even if no Fourier models were fitted. The full table is available at the CDS.