Peculiar velocities of galaxy clusters in a IllustrisTNG simulation based on mock observations of Sunyaev-Zel’dovich effects

Open Access

Fig. 13.

Distribution of |v_z, kSZ − v_z, halo| against the SFR of galaxy clusters in our sample for measurements with R_aper = R₂₀₀. The dashed line represents the rms scatter (∼55.15 km s⁻¹) of the v_z, kSZ = v_z, halo line at a given x-axis for all galaxy clusters based on measurements using apertures of R₂₀₀, as shown in Figure 8.

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.