Typical ASAS-SN V-band photometry. Top row: ASAS-SN normalized V-band photometry of asteroid (130) Elektra as a function of time (left) and phase angle α (right). Bottom row: comparison between the observed data and the model for asteroid (130) Elektra as a function of phase angle α (left) and the fit residuals with respect to the phase function f(α) (right). The actual H_V values are not relevant for our study, and therefore the relative flux is used instead.