  Mixed modes seen in evolved stars carry information on their deeper layers
that can place stringent constraints on their physics and on their global
properties (mass, age, etc...). In this study, we present a method to identify
and measure all oscillatory mode characteristics (frequency, height, width).
Analyzing four subgiants stars, we present the first measure of the effect of
the degree of mixture on the l=1 mixed modes characteristics. We also show that
some stars have measurable l=2 mixed modes and discuss the interest of their
measure to constrain the deeper layers of stars.
