Since no one answered, I would like to post here some useful insights on the matter.
The first, and most important, insight is that the improper uniform is inherently non-local. Distributions like Dirac's Delta, $\delta(t)$, have a local behavior, which is important. This issue makes the mathematical formalization of $\mathcal{K}(t)$ harder than it may appear.
The second comment is an attempted definition is the following. Consider the so-called integral mean (or average) over an interval $[a,b]$, given by
$$
\frac{1}{|a-b|} \int^b_{a} f(t) dt
$$
which is well-defined as long as the function $f$ is well-behaved. We can consider the limit of a sequence of increasing symmetric intervals as the mean of the function itself, given by
$$
\mathbb{E}[f] \triangleq \lim_{N \rightarrow +\infty} \frac{1}{2N} \int^N_{-N} f(t)dt
$$
and use this as our definition. In other words, the improper uniform can be thought of as an operator associating a real number to a function, i.e., $\mathbb{E} : \mathcal{F} \rightarrow \mathbb{R}$, where $\mathcal{F}$ is some function space with some regular properties (e.g.
Schwartz space). This approach can likely be refined significantly, but I invite the author to post his answer since, as of now, no better definition has been given (unfortunately, the bounty expired).
There is, however, one significant aspect which I think can be improved upon. Intuition tells us that $\mathcal{K}(t)$ should be an infinitesimally thin "carpet", spread over $\mathbb{R}$. So, it makes sense that it should share some properties of the zero-function (the pointwise limit of gaussians for $\sigma^2 -> +\infty$). This can be accomplished via the following definition
$$
\int_{\mathbb{R}} \mathcal{K}(t) f(t) dt = \lim_{\sigma^2 \rightarrow +\infty} \frac{1}{\sqrt{2 \pi \sigma^2}} \int_{\mathbb{R}} e^{-\frac{t^2}{2 \sigma^2}} f(t) dt
$$
Let us have a deeper look at this. For $f(t)=1$, we have that the result is $1$, so that
$$
\int_{\mathbb{R}} \mathcal{K}(t)dt = 1
$$
is satisfied. Consider now $f(t)=t$, for which the integral on the LHS is zero. This is, intuitively, correct, as $\mathcal{K}(t)$ should behave like the zero-function and simply make the integral vanish, but not always! We should expect some functions, like $f(t)=c$, for any $c \neq 0$, not to be annihilated. Functions with divergences also may be into this category. In other words, the integral is zero for some (but not all!) functions $f$, making $\mathcal{K}(t)$ "look like" the zero-function. To be more precise, there exists a function space $\mathcal{F}_0 \subsetneq \mathcal{F}$, where $\mathcal{F} = \mathcal{F}(\mathbb{R})$ is the space of all functions in $\mathbb{R}$ (regular enough to have an integral), such that
$$
\forall f \in \mathcal{F}_0: \quad \int_{\mathbb{R}} \mathcal{K}(t) f(t)dt = 0
$$
which means that $\mathcal{K}(t)$ acts like the zero-measure in $\mathcal{F}_0$. But, and this is the key point, it acts nontrivially when other functions ($\not\in \mathcal{F}_0$) come into play.
Look at this example. Call $\mathcal{K}(t)$ the improper uniform, with $t \in \mathbb{R}$ dummy variable (as in $\delta(t)$). Now, what is $$ \int_{\mathbb{R}} \mathcal{K}(t) f(t) dt = ? $$ where $f$ is your favorite well-behaved function, say $e^{- t^2}$. What does your intuition tell about that?
– PseudoRandom Feb 18 '18 at 12:11In an intuitive sense, you have that $\mathcal{K}(t) = dt$ for any $t$, i.e., a function of infinitesimal height whose integral is 1. It may be possible to give sense to $$ \int_{\mathbb{R}} \mathcal{K}(t)dt = \int_{\mathbb{R}} dt dt = \int_{\mathbb{R}} (dt)^2 = 1 $$ which, for now, is only empty formalism.
– PseudoRandom Feb 18 '18 at 14:07