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 .