The first law of black hole mechanics (let's simplify by considering a uncharged and non-rotating black hole) can be written as
$$\delta M = T \delta S$$
If I use the definition of Hawking temperature as $T=\frac{\kappa}{2 \pi}$ ($\kappa$=surface gravity) and entropy as $S=\frac{A}{4}$ ($A$=horizon area) then I can write this as
$$\delta M = \frac{\kappa \delta A}{8 \pi G}$$
Now this makes sense since the mass is essentially a conserved charge which I should get by some kind of Noether-like procedure where the conserved current is the stress tensor and if the Einstein-Hilbert term in my Lagrangian is $\mathcal{L}=-\frac{1}{16 \pi G}R$, then the stress-tensor (and thus $M$) will automatically come with the $8 \pi G$ to balance things out.
My question is to do with what happens if I use units in which the Einstein-Hilbert term of the Lagrangian is $\mathcal{L}=-\frac{1}{2}R$. This will rescale the stress-tensor (and consequently $M$) by $8 \pi G$ and so the factor of $\frac{1}{8 \pi G}$ on the right hand side needs to be removed. At first glance it seems quite straightforward: I can send $S \rightarrow A$ and $T \rightarrow \kappa$ so that my first law now reads $\delta M = \kappa \delta A$ like I want it to.
However, doesn't this affect dimensional analysis? Why have I never seen entropy or temperature defined like this in the literature? It seems a bit strange...