One of the activities foreseen within the D-NEAs project are photometric observations of asteroids that will be carried out from the Astronomical Station of Vidojevica. The primary purpose of this activity will be to collect information needed for our Monte Carlo model of surface thermal properties.
We will perform a multi-band photometry to determine the colors and the light- and phase curves. From the latter two, we will derive spin periods and absolute magnitudes of selected targets.