Left panel: planet radius as a function of stellar mass. The orange points indicate planets in multiple systems and the blue points are single planet systems. The dashed lines separates the smaller planets at 0.6 R_J from giant planets. Right panel: planetary mass (in logarithmic scale) as function of stellar mass. The dashed grey lines separates the low-mass planets at 0.2 M_J from giant planets. The black lines represent the linear fits with their Pearson Correlation Coefficients between planetary mass and radius with stellar mass for giant planets (solid black line) and low-mass planets (dashed black line).