Why are wavelengths shorter than visible light neglected by new telescopes? The diagram below, which I stole from this post by @HDE226868, shows that angular resolution as a function of wavelength suddenly drops by three orders of magnitudes from visible to UV-light. The resolution of wavelengths shorter than what the Very Large Telescope Interferometer or the European Extremely Large Telescope detect, in the near UV, suddenly cuts off to a factor of a thousand.

This is obviously because of the properties of Earth's atmosphere. But major space telescopes like the JWST and WFIRST will fill in the far infrared gap. Why aren't there any as ambitious space telescopes planned for UV and shorter wavelengths? (Or is the sudden cut off in that diagram misleading?)

Is it because it is more difficult, even from in-space observatories, or is it because the angular resolution of UV and shorter wavelengths are of lesser scientific value?
There are some technological issues to solve with putting any large telescope into space - and a space telescope is required at UV wavelengths. It is not possible to optimise such an instrument to work at both UV and IR wavelengths because of issues like cooling, mirror coatings and such-like. The simple angular resolution limit of a telescope goes $\lambda/D$, so on the face of it, to get equivalent resolution to an optical telescope, a UV telescope can be smaller. However, you also have to have optics that are good to a small fraction of a wavelength, so much better than the visible/IR. At even shorter wavelengths then conventional "optics" doesn't work because photons get absorbed and you move to the grazing incidence technologies of X-ray telescopes, which is a whole different game and much harder to achieve a given angular resolution.

Given all that, back in the 80s/90s I would guess that a decision was taken about the wavelength range to be covered by the successor to HST (ie JWST at a cost of approximately 10 billion USD) The real reason that no major UV successor to HST or IUE is ready to go now is simply that it is considered that the most important science priorities are achievable at near and mid-IR wavelengths. These are: observing the high redshift universe (essentially no UV light is detected from galaxies beyond a redshift of 3), observing star and planet formation (mostly in dusty environments where UV light cannot emerge and protoplanetary discs emit mostly at IR wavelengths) and doing exoplanetary science (planets are cooler than stars and emit mostly in the IR).

Thus, I don't think there are any technological showstoppers to a big UV telescope (at least the equivalent of JWST), it just comes down to science prorities.