A classical-light time-to-space ghost imaging scheme achieves sub-picosecond temporal resolution independent of photodetector response time via Gaussian Schell model analysis and a grating-plus-SLM source.
How- ever, the same effect can be reached in the near field of the disk [52], in which case the coherence length is fixed to the average size of the disk inhomogeneities
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Time-to-space ghost imaging with classical light
A classical-light time-to-space ghost imaging scheme achieves sub-picosecond temporal resolution independent of photodetector response time via Gaussian Schell model analysis and a grating-plus-SLM source.