In these lecture notes by Strominger section 3.3 we derive the equations of motion of the Classical Dilaton Gravity action $$ S = \frac{1}{2\pi}\int{d^2x}{\sqrt{-g}e^{-2\phi}\left(R +4 (\nabla\phi)^2+4\lambda^2\right)}\tag{3.6} $$
The equations of motion for the metric are $$ 2 e^{-2\phi}(\nabla_\mu\nabla_\nu\phi+g_{\mu\nu}((\nabla\phi)^2-\nabla^2\phi-\lambda^2)=0\tag{3.7} $$
Then by introducing light-cone coordinates and gauge fixing the metric we have $$ g_{+-}=-\frac{1}{2}e^{2\rho}\qquad g_{++}=g_{--}=0\tag{3.12} $$
Finally for the $g_{++}$ and $g_{--}$ the equations of motion in terms of the light-cone coordinates give $$ e^{-2\phi}(4\partial_+\rho\partial_+\phi-2\partial_+^2\phi)=0 \\e^{-2\phi}(4\partial_-\rho\partial_-\phi-2\partial_-^2\phi)=0\tag{3.15} $$
I don't understand where the last 2 equations come from. Are they not supposed to be the components $_{++}$ and $_{--}$ of the equation of motion of the metric found before?