Using multiobjective optimization to reconstruct interferometric data (I)
arXiv:2304.12107 · doi:10.1051/0004-6361/202346207
Abstract
Imaging in radioastronomy is an ill-posed inverse problem. Particularly the Event Horizon Telescope (EHT) Collaboration investigated the fidelity of their image reconstructions convincingly by large surveys solving the problem with different optimization parameters. This strategy faces a limitation for the existing methods when imaging the active galactic nuclei (AGN): large and expensive surveys solving the problem with different optimization parameters are time-consumptive. We present a novel nonconvex, multiobjective optimization modeling approach that gives a different type of claim and may provide a pathway to overcome this limitation. To this end we used a multiobjective version of the genetic algorithm (GA): the Multiobjective Evolutionary Algorithm Based on Decomposition, or MOEA/D. GA strategies explore the objective function by evolutionary operations to find the different local minima, and to avoid getting trapped in saddle points. First, we have tested our algorithm (MOEA/D) using synthetic data based on the 2017 Event Horizon Telescope (EHT) array and a possible EHT + next-generation EHT (ngEHT) configuration. We successfully recover a fully evolved Pareto front of non-dominated solutions for these examples. The Pareto front divides into clusters of image morphologies representing the full set of locally optimal solutions. We discuss approaches to find the most natural guess among these solutions and demonstrate its performance on synthetic data. Finally, we apply MOEA/D to observations of the black hole shadow in Messier 87 (M87) with the EHT data in 2017. MOEA/D is very flexible, faster than any other Bayesian method and explores more solutions than Regularized Maximum Likelihood methods (RML).
arXiv commentto appear in A&A
References in corpus (17)
- First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole
- A multi-scale multi-frequency deconvolution algorithm for synthesis imaging in radio interferometry
- Multi-Scale CLEAN deconvolution of radio synthesis images
- First Sagittarius A* Event Horizon Telescope Results. III: Imaging of the Galactic Center Supermassive Black Hole
- High Resolution Linear Polarimetric Imaging for the Event Horizon Telescope
- Interferometric Imaging Directly with Closure Phases and Closure Amplitudes
- Imaging the Schwarzschild-radius-scale Structure of M87 with the Event Horizon Telescope using Sparse Modeling
- Super-resolution Full Polarimetric Imaging for Radio Interferometry with Sparse Modeling
- Scale sensitive deconvolution of interferometric images I. Adaptive Scale Pixel (Asp) decomposition
- Dynamical Imaging with Interferometry
- Closure statistics in interferometric data
- Hybrid Very Long Baseline Interferometry Imaging and Modeling with Themis
- Comparison of classical and Bayesian imaging in radio interferometry
- Spurious source generation in mapping from noisy phase-self-calibrated data
- Multi-scale and Multi-directional VLBI Imaging with CLEAN
- Dynamic and polarimetric VLBI imaging with a multiscalar approach
- A first search of transients in the Galactic Center from 230 GHz ALMA observations
Cited by in corpus (11)
- Bayesian self-calibration and imaging in Very Long Baseline Interferometry
- Imaging a ring-like structure and the extended jet of M87 at 86 GHz
- Event-horizon-scale Imaging of M87* under Different Assumptions via Deep Generative Image Priors
- Swarm intelligence for full Stokes dynamic imaging reconstruction of interferometric data
- Deep learning inference with the Event Horizon Telescope II. The Zingularity framework for Bayesian artificial neural networks
- Prospects of using closure traces directly for imaging in Very Long Baseline Interferometry
- How to make CLEAN variants faster? Using clustered components informed by the autocorrelation function
- Probing circular polarization and magnetic field structure in AGN
- Accelerating the CLEAN algorithm of radio interferometry with convex optimization
- Very-Long Baseline Interferometry Imaging with Closure Invariants using Conditional Image Diffusion
- Multiobjective optimization for scattering mitigation and scattering screen reconstruction in VLBI observations of the Galactic Center