Asteroid families detected within the MOVIS catalog, with at least 40 coincidences with NEOWISE, and with a background of at least ten asteroids. In these plots we represent ML^* vs. p_NIR. On the left, we represent the observed family, and on the right the background we defined for that same family. Upper plots are weighted density plots (see text for explanation), and lower plots are scatter representations of the observed asteroids, with the corresponding error bars.