Logarithmic slope of total transit depth
= Logarithmic slope of total transit depth
For $\delta=A+B(1-e^{-\tau})$ and $\tau\propto\lambda^{-p}$, the logarithmic slope is $-pB\tau e^{-\tau}/\delta$. The opaque planetary baseline generally dilutes the slope. In the <optically thin> limit, the atmospheric excess $\delta-A$ has logarithmic slope $-p$.