Graduate Stumped by a Lagrangian in Einstein's 1916 paper

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Struggling to match the E-L equations from an assumed Lagrangian
I decided recently that I would work through Einstein's original paper on the foundation of GR and I've recently hit a roadblock. It starts with Einstein's Lagrangian for an empty space-time,

$$ \begin{align} \mathcal{L}= g^{\mu \nu} \Gamma^{\alpha}_{\nu \beta} \Gamma^{\beta}_{\mu \alpha} \tag{47a} \end{align}, $$

which, Einstein shows, gives the two quantities:

$$ \begin{align*} \frac{\partial \mathcal{L}}{\partial g^{\mu\nu}} = - \Gamma^{\alpha}_{\mu \beta} \Gamma^{\beta}_{\nu \alpha}; \\
\frac{\partial \mathcal{L}}{\partial (\partial_\sigma g^{\mu\nu})} = \Gamma^{\sigma}_{\mu \nu}. \tag{48} \end{align*} $$

I can follow the maths as given in the paper to arrive at this result, but I am confused by the first step. Namely, ##\mathcal{L}## is a function of ##(g^{\mu\nu}, \partial_\sigma g^{\mu\nu})##, yet it is differentiated wrt ## (g^{\mu\nu}, \Gamma^{\beta}_{\nu\alpha}).## But isn't ##\Gamma## a function of both ##(g^{\mu\nu}, \partial_\sigma g^{\mu\nu})##? When I differentiate wrt to these, I get the following quantities:

$$ \begin{align*}
\mathcal{L}(g^{\mu \nu}, \partial_\rho g^{\mu \nu}) &= g^{\sigma \tau} \Gamma^{\alpha}_{\sigma \beta} \Gamma^{\beta}_{\tau \alpha}; \\
\delta \mathcal{L} &= \left[ \Gamma^{\alpha}_{\sigma \beta} \Gamma^{\beta}_{\tau \alpha} + 2g^{\sigma\tau}\frac{\partial \Gamma^\alpha_{\sigma\beta}}{\partial g^{\mu\nu}} \right]\delta(g^{\mu\nu}) + 2\left[g^{\sigma\tau}\Gamma^{\alpha}_{\sigma\beta}\frac{\partial \Gamma^{\beta}_{\tau\alpha}}{\partial(\partial_\rho g^{\mu\nu})} \right]\delta(\partial_\rho g^{\mu\nu});\\
\frac{\partial \mathcal{L}}{\partial g^{\mu\nu}} &= 3\Gamma^{\alpha}_{\mu \beta} \Gamma^{\beta}_{\nu \alpha}; \\
\frac{\partial \mathcal{L}}{\partial (\partial_\sigma g^{\mu\nu})} &= \Gamma^{\sigma}_{\mu \nu}.
\end{align*}
$$

I guess my main question is, why are we disregarding the ## g^{\mu\nu}## dependency in ##\Gamma##? I trace the difference to the second term in the first square bracket: if its sign were different, I would obtain the same answer! Thanks.

(Here's a link to the paper for ease of access ^^: https://en.wikisource.org/wiki/The_Foundation_of_the_Generalised_Theory_of_Relativity#§_15._Hamiltonian_Function_for_the_Gravitation-field._Laws_of_Impulse_and_Energy.)
 
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MOVING CLOCKS In this section, we show that clocks moving at high speeds run slowly. We construct a clock, called a light clock, using a stick of proper lenght ##L_0##, and two mirrors. The two mirrors face each other, and a pulse of light bounces back and forth betweem them. Each time the light pulse strikes one of the mirrors, say the lower mirror, the clock is said to tick. Between successive ticks the light pulse travels a distance ##2L_0## in the proper reference of frame of the clock...

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