Optimized Image Reconstruction: Insights from Optical Interferometry

          @misc{ scivideos_PIRSA:14110072,
            doi = {10.48660/14110072},
            url = {https://pirsa.org/14110072},
            author = {Monnier, John},
            keywords = {Strong Gravity},
            language = {en},
            title = {Optimized Image Reconstruction: Insights from Optical Interferometry},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2014},
            month = {nov},
            note = {PIRSA:14110072 see, \url{https://scivideos.org/pirsa/14110072}}
          }
          

Abstract

The radio community pioneered the use of closure phases to allow interferometric imaging even when fringe phases are compromised by atmospheric turbulence or unstable reference clocks. Eventually, better receivers and observing methods allowed phase referencing to provide direct measures of complex visibilities and eased the uncertainties using Fourier inversions required for imaging. At the same time, optical and infrared (O/IR) interferometers have been developed recently that can combine up to 6 telescopes simultaneously, at which point the inadequacies of classic imaging methods such as CLEAN were apparent. Here I report on dramatic progress within the O/IR interferometry to develop new image reconstruction techniques taking advantage of advances in ``compressed sensing'' theory and new approaches afforded by modern computing. Because the Event Horizon Telescope must rely on closure phases instead of direct Fourier phases, the new algorithms from the O/IR could be essential to extracting the most information from EHT observations and we demonstrate promising results using simulated EHT data.