Oh Dear.
Most of the exoplnaets discovered so far have been supermassive 'hot Jupiters', that is gas giants larger than Jupiter which orbit very close to their parent star (e.g. well within the orbit of Mercury). This is because the easiest method of detecting exoplanets is the 'wobble' caused by the orbits of such planets.
Smaller gas planets (such as Neptune) are harder to spot, as are planets orbiting further from their star, as these can only really be spotted when they transit (cross in formt of their parent star), which requires that they orbit in a plane that brings them between us and their parent star.
Small rocky planets, such as Earth are even harder still to spot, with ther discovery requiring methods such as looking for changes in their prent star's emission spectrum when they transit, as their size will mean that they hardly affect the amount of light reaching Earth at all.
Having said all that, what these researchers seem to have found is that there is some sort of relationship between close-orbiting large gas giants and low amounts of lithium in a star. Extrapolating this to draw a parallel between the existence of any sort of planetary system and observable lithium levels in a star's emission spectrum seems to be stretching it a little.