Properties of the magnetic topologies for cool, main-sequence stars obtained via ZDI. The locations of StKM 1-1262 and V374 Peg are highlighted. The y- and x-axes represent the mass and rotation period of the star. Gray curves illustrate different Rossby numbers (Ro = 0.01, 0.1 and 1.0), and are obtained using the empirical relations of Wright et al. (2018). The Rossby number is the ratio between the rotation period of a star and the convective turnover time. The symbol size, colour, and shape encodes the ZDI average field strength, poloidal/toroidal energy fraction, and axisymmetry (see Petit et al. 2008; Morgenthaler et al. 2012; Fares et al. 2013; Boro Saikia et al. 2015; do Nascimento et al. 2016; Boro Saikia et al. 2016; Hussain et al. 2016; Alvarado-Gómez et al. 2015; Folsom et al. 2016, 2018; Kochukhov & Shulyak 2019; Folsom et al. 2020; Klein et al. 2021; Willamo et al. 2022; Martioli et al. 2022; Bellotti et al. 2023a; Lehmann et al. 2024, for the data used). For stars with multiple reconstructions, the data represent the most recent ZDI maps.