Corner plot showing the time-weighted distributions of the properties of wind-fed BH-HMXBs from the moderately super-Eddington accretion scenario. The dark and light blue contours represent the 68% and 95% confidence regions, respectively, for the orbital period, donor star mass, BH mass, BH spin, and X-ray luminosity of systems after RLO. Similarly, the dark and light orange contours are for systems before RLO. The black dot, square, and triangle with error bars indicate the positions of Cygnus X-1, LMC X-1, and M33 X-7, respectively.