LPA caracterisation for G2 stars (left) and K2 stars (right). First row: distribution of the LPA detection limits for ΔT_spot1 (solid lines) and ΔT_spot2 (dashed lines) for the different HZ periods: lower HZ (black), medium HZ (red), and upper HZ (green). Third row: same for the distribution of the detection rates corresponding to the LPA masses. Fourth row: same for the distribution of exclusion rates corresponding to the LPA masses.