I've been teaching myself relativity by reading Sean Carroll's intro to General Relativity textbook, and in the first chapter he discusses special relativity and introduces the concept of tensors, which I am still very new to. Near the end of the chapter, he introduces the electromagnetic field strength tensor: $$ F_{\mu\upsilon} = \left( \begin{matrix} 0 & -E_1 & -E_2 & -E_3\\ E_1 & 0 & B_3 & -B_2\\ E_2 & -B_3 & 0 & B_1\\ E_3 & B_2 & -B_1 & 0\\ \end{matrix} \right) = -F_{\upsilon\mu}$$
He then writes the four Maxwell equations in tensor notation, using the elements of the above field tensor: $$ \bar{\epsilon}^{ijk}\partial_jB_k - \partial_0E^i = J^i\\ \partial_iE^i = J^0\\ \bar{\epsilon}^{ijk}\partial_jE_k + \partial_0B^i = 0\\ \partial_iB^i = 0.$$ Next, by showing that the field tensor can be represented by the two tensor equations $F^{0i} = E^i$ and $F^{ij} = \bar{\epsilon}^{ijk}B_k$, he proposes that the first two of Maxwell's equations can be written as: $$ \partial_jF^{ij} - \partial_0F^{0i} = J^i\\ \partial_iF^{0i} = J^0$$ Finally, he proposes that by using the antisymmetry of $F_{\mu\upsilon}$, the above two equations can be reduced to the single equation: $$ \partial_\mu F^{\upsilon\mu} = J^{\upsilon}$$ My question is, can someone show me how to use the antisymmetry of $F_{\mu\upsilon}$ to derive the last equation from the penultimate pair of equations? Note that in this context, $J$ is the current 4-vector in Gaussian form, $J = (\rho, J^x, J^y, J^z)$, $\bar{\epsilon}^{ijk}$ is the Levi-Civita symbol in spatial coordinates, and Latin subscripts and superscripts refer to spatial coordinates while Greek subscripts and superscripts refer to spacetime coordinates.