There are many reasons why we see macroscopic electromagnetic waves, but not electron waves of the same sort (i.e. free traveling in space). First and foremost, electrons have charge and photons don't, so it takes a lot of energy to isolate them from ions and send them free streaming through space.
Second, electrons have mass and photons don't. Because of this, for any given kinetic energy
\begin{align}
K_e & \equiv \sqrt{(m_ec^2)^2 + \left(\frac{hc}{\lambda_e}\right)^2} - mc^2 = \frac{\left(\frac{hc}{\lambda_e}\right)^2}{m_ec^2 + \sqrt{(m_ec^2)^2 + \left(\frac{hc}{\lambda_e}\right)^2}}\ \mathrm{and} \\
K_\gamma & \equiv \frac{hc}{\lambda_\gamma} ,\ \Rightarrow \\
\lambda_e & = \frac{hc}{\sqrt{2K_e m_e c^2 + K_e^2}}\ \mathrm{and} \\
\lambda_\gamma &= \frac{hc}{K_\gamma},
\end{align}
thus $\lambda_e < \lambda_\gamma$, always. For example, at room temperature, $T\approx 300K \Rightarrow \lambda_\gamma\sim 10\operatorname{\mu m},\ \lambda_e \sim 3 \operatorname{nm}$, and when $\lambda_\gamma=1\operatorname{m},\ \lambda_e = 1.101 \operatorname{\mu m}$. In other words, to get $\lambda_e\sim 1\operatorname{m}$, you'd need temperatures $T\sim 4\times10^{-15}\operatorname{K}$ or less in your detectors and in the space the electron is passing through (otherwise a photon blackbody will heat it).
Note that this is why electron microscopes have such good resolution.
Third, electrons are fermions and photons are bosons. This isn't obviously relevant, but when you actually want to detect a macroscopic wave, it helps if you have an Avogadro's number (or more) of particles to give the wave plenty of energy to detect. A low energy, long wavelength electron, because of the Pauli exclusion principle, will always be solo, or require a prohibitively large space to get enough similar wavelength modes near each other, and so it's harder to detect. In comparison, it's actually tricky to get singleton low energy Bosons (correct me if I'm wrong, but I've never heard of people working with centimeter plus wavelength photons that weren't in waves with massive numbers of them).
Long story short, the best you're likely to be able to do with electrons is the sort of charge density waves studied in magnetohydrodynamics, antenna design, wave guides, beam physics (especially in free electron lasers), surface plasmons, etc. In other words, electron waves are usually either microscopic or confined to a region of space by being bound to a conductor or plasma, for practical reasons.
