Hi Gheorghe,
Thanks for reading my essay and as well the journal paper which was the basis of the first part of the essay.
In regard to your question " Is the measurement of the Unruh versus Hawking temperature and correlations that you describe in any way different from the situation described above?"
My contention is that it is different. The Unruh-DeWitt allows one to make local measurements of the temperature and transition rate. The physical picture I like to keep in mind for the UD detector is an electron in a magnetic field. This has two states and one can measure the rate at which the upper state gets excited in a particular space-time (e.g. Schwarzschild) or for a particular space-time path (Rindler observer). The conceptual reason for why the local measurement with an UD detector can obtain global information about the space-time or space-time path is that its transition rate depends on the field modes which depend on the global structure of the space-time or space-time path. Also QM in general has non-local features (such as entanglement) and the EP is local.
The question of shielding the radiation is interesting and I have not fully understood this. Certainly, under normal circumstances, one can shield the UD detector from Hawking radiation (By "under normal conditions" I mean at all points in the BH evaporation process except at the very end when it will emit gamma rays of increasingly high energy and short wavelength. At some point the wavelengths of the gamma ray photons emitted by the small BH will be much smaller than the interatomic spacing and it will not be possible to shield them).
On the other hand I am not sure if it is at all possible to shield an UD detector from Unruh radiation.
Best,
Doug