VELOCE modulation zoo. III.

X Sagittarii exhibited dominant additional signals, notably one at approximately 12.31 days, also associated with significant line splitting. Polaris revealed multiple low-frequency signals, with the most prominent candidate at approximately 59.86 days, which might be linked to the rotation period of the star. We explored the semi-partial distance correlation periodograms by incorporating cross-correlation functions (CCFs) and their variants, such as the median-subtracted CCFs, which improved sensitivity to line shape variations.

In particular, the latter enabled the faithful detection of primary and additional signals present in the 1D spectra of fainter stars and low-amplitude pulsators. The semi-partial distance correlation periodograms demonstrated their utility for isolating signals associated with line shape variations although the analyses were complicated by the presence of artefact subharmonics and a visible low-frequency power increase for Polaris and BG Crucis.

This study underscores the potential of the method for finding new and unexpected signals as well as detailed analyses of Cepheid pulsations and opens new pathways for asteroseismic investigations.