Extended Data Fig. 3: Δi as a function of adopted system properties.
From: One-third of Sun-like stars are born with misaligned planet-forming disks
a–h, Δi as a function of: spectral type, M*, Teff, R*, Prot, vsini*, idisk and i*. Pearson r correlation coefficients and their respective P-values are shown in the upper left of each cell. Data points within each panel are split into two subpopulations that are used to test for parameter-dependent clustering in Δi (see Methods) and are shown here in purple (subgroup 1) and pink (subgroup 2). The mean values and standard deviations for groups 1 and 2 are shown in each panel and the significance level of the difference between subgroups (σ) is also shown in each panel. Error bars are shown at 1σ confidence.
