  We present physical models, i.e. convex shapes, directions of the rotation
axis, and sidereal rotation periods, of 18 asteroids out of which 10 are new
models and 8 are refined models based on much larger data sets than in previous
work. The models were reconstructed by the lightcurve inversion method from
archived publicly available lightcurves and our new observations with
BlueEye600 robotic observatory. One of the new results is the shape model of
asteroid (1663)~van~den~Bos with the rotation period of 749\,hr, which makes it
the slowest rotator with known shape. We describe our strategy for target
selection that aims at fast production of new models using the enormous
potential of already available photometry stored in public databases. We also
briefly describe the control software and scheduler of the robotic observatory
and we discuss the importance of building a database of asteroid models for
studying asteroid physical properties in collisional families.
