Dynamical Imaging with Interferometry
arXiv:1711.01286 · doi:10.3847/1538-4357/aa97dd
Abstract
By linking widely separated radio dishes, the technique of very long baseline interferometry (VLBI) can greatly enhance angular resolution in radio astronomy. However, at any given moment, a VLBI array only sparsely samples the information necessary to form an image. Conventional imaging techniques partially overcome this limitation by making the assumption that the observed cosmic source structure does not evolve over the duration of an observation, which enables VLBI networks to accumulate information as the Earth rotates and changes the projected array geometry. Although this assumption is appropriate for nearly all VLBI, it is almost certainly violated for submillimeter observations of the Galactic Center supermassive black hole, Sagittarius A* (Sgr A*), which has a gravitational timescale of only ~20 seconds and exhibits intra-hour variability. To address this challenge, we develop several techniques to reconstruct dynamical images ("movies") from interferometric data. Our techniques are applicable to both single-epoch and multi-epoch variability studies, and they are suitable for exploring many different physical processes including flaring regions, stable images with small time-dependent perturbations, steady accretion dynamics, or kinematics of relativistic jets. Moreover, dynamical imaging can be used to estimate time-averaged images from time-variable data, eliminating many spurious image artifacts that arise when using standard imaging methods. We demonstrate the effectiveness of our techniques using synthetic observations of simulated black hole systems and 7mm Very Long Baseline Array observations of M87, and we show that dynamical imaging is feasible for Event Horizon Telescope observations of Sgr A*.
16 Pages, 12 Figures, Accepted for publication in ApJ
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Cited by in corpus (49)
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- Reference Array and Design Consideration for the next-generation Event Horizon Telescope
- Superresolution Interferometric Imaging with Sparse Modeling Using Total Squared Variation --- Application to Imaging the Black Hole Shadow
- The Varying Kinematics of Multiple Ejecta from the Black Hole X-ray Binary MAXI J1820+070
- Metrics and Motivations for Earth-Space VLBI: Time-Resolving Sgr A* with the Event Horizon Telescope
- Test of Einstein equivalence principle near the Galactic center supermassive black hole
- HI 21cm Cosmology and the Bi-spectrum: Closure Diagnostics in Massively Redundant Interferometric Arrays
- Studying Black Holes on Horizon Scales with VLBI Ground Arrays
- Simulations of M87 and Sgr A* Imaging with the Millimetron Space Observatory on near-Earth orbits
- Silhouettes of invisible black holes
- Selective Dynamical Imaging of Interferometric Data
- Using space-VLBI to probe gravity around Sgr A*
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- Black hole parameter estimation with synthetic Very Long Baseline Interferometry data from the ground and from space
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- Black hole Spin Measurement Based on Time-domain VLBI Observations of Infalling Gas Cloud
- Wideband Super-resolution Imaging in Radio Interferometry via Low Rankness and Joint Average Sparsity Models (HyperSARA)
- Principal Component Analysis as a Tool for Characterizing Black Hole Images and Variability
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- Dynamic and polarimetric VLBI imaging with a multiscalar approach
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- Prospects of using closure traces directly for imaging in Very Long Baseline Interferometry
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- Characterization of black hole accretion through image moment invariants
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