[guided]We now have coordinate limits $a_i \in \mathbb{R}$ for $i \in \{1,\dots,n\}$, and we have defined
\begin{align*}
a = (a_1,\dots,a_n) \in \mathbb{R}^n.
\end{align*}
To prove convergence in the Euclidean metric, we must prove that for every $\varepsilon>0$ there exists $M \in \mathbb{N}$ such that $m \ge M$ implies
\begin{align*}
d_2(x_m,a)<\varepsilon.
\end{align*}
Let $\varepsilon>0$. Since $n \in \mathbb{N}$ and the convention is that $\mathbb{N}$ starts at $1$, the number $\sqrt{n}$ is positive. For each coordinate $i \in \{1,\dots,n\}$, the real convergence $x_{m,i} \to a_i$ gives an integer $M_i \in \mathbb{N}$ such that for all $m \ge M_i$,
\begin{align*}
|x_{m,i}-a_i|<\frac{\varepsilon}{\sqrt{n}}.
\end{align*}
Because there are only finitely many coordinates, we can choose one index threshold that works for all of them:
\begin{align*}
M = \max\{M_1,\dots,M_n\}.
\end{align*}
Then $m \ge M$ implies $m \ge M_i$ for every $i \in \{1,\dots,n\}$, so every coordinate error satisfies
\begin{align*}
|x_{m,i}-a_i|<\frac{\varepsilon}{\sqrt{n}}.
\end{align*}
Substituting these coordinate bounds into the definition of the Euclidean metric gives
\begin{align*}
d_2(x_m,a)^2 = \sum_{i=1}^n |x_{m,i}-a_i|^2 < \sum_{i=1}^n \frac{\varepsilon^2}{n} = \varepsilon^2.
\end{align*}
The quantities $d_2(x_m,a)$ and $\varepsilon$ are non-negative, so taking square roots yields
\begin{align*}
d_2(x_m,a)<\varepsilon.
\end{align*}
This proves $x_m \to a$ in the metric $d_2$.[/guided]