Commodore, We only find "side view," or what astronomers refer to as edge on, systems because of our limited detection techniques. The two methods to regularly find planets so far are photometry and radial velocity. One relies on a faint dip in light when a planet passes in front of its star and the other relies on a planet pulling its star slightly towards it.
There's no reason to think that a universal preference would exist for solar systems facing us edge on. So, by simply taking an infrared photo of the star - similar to what Hubble did with Fomalhaut and NASA did here- we might determine the presence of a planet based on a dust cloud around it.