Imaging the Schwarzschild-radius-scale Structure of M87 with the Event Horizon Telescope using Sparse Modeling
arXiv:1702.07361 · doi:10.3847/1538-4357/aa6305
Abstract
We propose a new imaging technique for radio and optical/infrared interferometry. The proposed technique reconstructs the image from the visibility amplitude and closure phase, which are standard data products of short-millimeter very long baseline interferometers such as the Event Horizon Telescope (EHT) and optical/infrared interferometers, by utilizing two regularization functions: the -norm and total variation (TV) of the brightness distribution. In the proposed method, optimal regularization parameters, which represent the sparseness and effective spatial resolution of the image, are derived from data themselves using cross validation (CV). As an application of this technique, we present simulated observations of M87 with the EHT based on four physically motivated models. We confirm that +TV regularization can achieve an optimal resolution of % of the diffraction limit , which is the nominal spatial resolution of a radio interferometer. With the proposed technique, the EHT can robustly and reasonably achieve super-resolution sufficient to clearly resolve the black hole shadow. These results make it promising for the EHT to provide an unprecedented view of the event-horizon-scale structure in the vicinity of the super-massive black hole in M87 and also the Galactic center Sgr A*.
16 pages, 6 figures, accepted for publication in ApJ
References in corpus (14)
- Event-horizon-scale structure in the supermassive black hole candidate at the Galactic Centre
- Jet Launching Structure Resolved Near the Supermassive Black Hole in M87
- Compressed sensing imaging techniques for radio interferometry
- The old nuclear star cluster in the Milky Way: dynamics, mass, statistical parallax, and black hole mass
- Sparsity Averaging Reweighted Analysis (SARA): a novel algorithm for radio-interferometric imaging
- 230 GHz VLBI observations of M87: event-horizon-scale structure at the enhanced very-high-energy -ray state in 2012
- Imaging the Supermassive Black Hole Shadow and Jet Base of M87 with the Event Horizon Telescope
- LOFAR Sparse Image Reconstruction
- Super-resolution Full Polarimetric Imaging for Radio Interferometry with Sparse Modeling
- Imaging an Event Horizon: Mitigation of Scattering Toward Sagittarius A*
- MORESANE: MOdel REconstruction by Synthesis-ANalysis Estimators. A sparse deconvolution algorithm for radio interferometric imaging
- Compressed sensing for wide-field radio interferometric imaging
- Stochastic Optics: A Scattering Mitigation Framework for Radio Interferometric Imaging
- Doppler Tomography by Total Variation Minimization
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- RadioAstron discovery of a mini-cocoon around the restarted parsec-scale jet in 3C 84
- A Mechanism for Triple-Ridge Emission Structure of AGN Jets
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- Multi-scale and Multi-directional VLBI Imaging with CLEAN
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- Dynamic and polarimetric VLBI imaging with a multiscalar approach
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- CLEAN imaging systematics of M87 radio jet
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- exoALMA. VIII. Probabilistic Moment Maps and Data Products using Non-parametric Linear Models
- Lensing Signatures of a Slowly-Accelerated Black Hole
- Event-horizon-scale Imaging of M87* under Different Assumptions via Deep Generative Image Priors
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- A Jet Source of Event Horizon Telescope Correlated Flux in M87
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- Super-Resolved Image of M87 Observed with East Asian VLBI Network
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