The energy-momentum tensor $T^{\mu\nu}$ is not uniquely defined because we can add a term $\partial_{\lambda}X^{\lambda\mu\nu}$ to it, where $X^{\lambda\mu\nu} = - X^{\mu\lambda\nu}$, and show that it is still divergenceless.
I know $\partial{\mu}T^{\mu\nu} = 0$ because $T^{\mu\nu}$ is a conserved current. I also know that I should use the antisymmetry condition above along with the fact that the repeated indices need to be summed over.
I also know that $$\partial_{\nu}x^{\mu} \equiv \delta_{\nu}^{\mu} \tag{1}$$ and $$\partial_{\mu}x^{\mu} \equiv \delta_{\mu}^{\mu}=4\tag{2}$$ due to the number of spacetime dimensions in the problem.
Question: How would I explicitly be able to take the derivative of a tensor using index notation? I want to show the above statement, but I would also like to explicitly be able to calculate the term $\partial_{\mu}\partial_{\lambda}X^{\lambda\mu\nu}$. Is there a way to extend the definitions (1) and (2) above for taking derivatives / multiple derivatives of tensors?