VELOcities of CEpheids (VELOCE) - I. High-precision radial velocities of Cepheids

Open Access

Fig. 30

Differences between $v_{γ, G D R 3}^{⋆}$ $\[v_{\gamma, \mathrm{GDR} 3}^{\star}\]$ (template fits to Gaia RVs) and VELOCE υ_γ of 121 time clusters of 66 non-SB1 Cepheids where $| σ_{Δ v_{γ}} | \leq 0.5 k m s^{- 1}$ $\[\left|\sigma_{\Delta v_\gamma}\right| \leq0.5 \mathrm{~km} \mathrm{~s}^{-1}\]$ . Horizontal errorbars indicate the duration of the time series used for the fit, vertical errorbars show the uncertainty of the velocity difference. The median difference is 0.65 ± 0.11 km s⁻¹.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.