PAINTER: a spatio-spectral image reconstruction algorithm for optical interferometry
arXiv:1407.1885 · doi:10.1364/JOSAA.31.002334
Abstract
Astronomical optical interferometers sample the Fourier transform of the intensity distribution of a source at the observation wavelength. Because of rapid perturbations caused by atmospheric turbulence, the phases of the complex Fourier samples (visibilities) cannot be directly exploited. Consequently, specific image reconstruction methods have been devised in the last few decades. Modern polychromatic optical interferometric instruments are now paving the way to multiwavelength imaging. This paper is devoted to the derivation of a spatio-spectral (3D) image reconstruction algorithm, coined PAINTER (Polychromatic opticAl INTErferometric Reconstruction software). The algorithm relies on an iterative process, which alternates estimation of polychromatic images and of complex visibilities. The complex visibilities are not only estimated from squared moduli and closure phases, but also differential phases, which helps to better constrain the polychromatic reconstruction. Simulations on synthetic data illustrate the efficiency of the algorithm and in particular the relevance of injecting a differential phases model in the reconstruction.
12 pages, 10 figures, http://www.opticsinfobase.org/submit/review/copyright_permissions.cfm
References in corpus (4)
- Monte-Carlo Imaging for Optical Interferometry
- SPARCO : a semi-parametric approach for image reconstruction of chromatic objects
- VLTI/AMBER differential interferometry of the broad-line region of the quasar 3C273
- A scene model of exosolar systems for use in planetary detection and characterisation simulations
Cited by in corpus (6)
- Principles of image reconstruction in optical interferometry: tutorial
- Proximity Operators for Phase Retrieval
- Why Chromatic Imaging Matters
- TLDR: Time Lag/Delay Reconstructor
- Back-propagating the light of field stars to probe telescope mirrors aberrations
- Large Scale 3D Image Reconstruction in Optical Interferometry