Variable structures in M87* from space, time and frequency resolved interferometry
arXiv:2002.05218 · doi:10.1038/s41550-021-01548-0
Abstract
Observing the dynamics of compact astrophysical objects provides insights into their inner workings, thereby probing physics under extreme conditions. The immediate vicinity of an active supermassive black hole with its event horizon, photon ring, accretion disk, and relativistic jets is a perfect place to study general relativity and magneto-hydrodynamics. The observations of M87* with Very Long Baseline Interferometry (VLBI) by the Event Horizon Telescope (EHT) allows to investigate its dynamical processes on time scales of days. Compared to regular radio interferometers, VLBI networks typically have fewer antennas and low signal to noise ratios (SNRs). Furthermore, the source is variable, prohibiting integration over time to improve SNR. Here, we present an imaging algorithm that copes with the data scarcity and temporal evolution, while providing uncertainty quantification. Our algorithm views the imaging task as a Bayesian inference problem of a time-varying brightness, exploits the correlation structure in time, and reconstructs a dimensional time-variable and spectrally resolved image at once. We apply this method to the EHT observation of M87* and validate our approach on synthetic data. The time- and frequency-resolved reconstruction of M87* confirms variable structures on the emission ring. The reconstruction indicates extended and time-variable emission structures outside the ring itself.
32 pages, 17 figures, 6 tables
References in corpus (8)
- First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
- First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole
- First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole
- First M87 Event Horizon Telescope Results. V. Physical Origin of the Asymmetric Ring
- First M87 Event Horizon Telescope Results. II. Array and Instrumentation
- First M87 Event Horizon Telescope Results. III. Data Processing and Calibration
- Dynamical Imaging with Interferometry
- Reconstruction of signals with unknown spectra in information field theory with parameter uncertainty
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- Key Science Goals for the Next-Generation Event Horizon Telescope
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- Reference Array and Design Consideration for the next-generation Event Horizon Telescope
- The Photon Ring in M87*
- Adaptive Analytical Ray Tracing of Black Hole Photon Rings
- Multi-frequency Black Hole Imaging for the Next-Generation Event Horizon Telescope
- When models fail: an introduction to posterior predictive checks and model misspecification in gravitational-wave astronomy
- Re-Envisioning Numerical Information Field Theory (NIFTy.re): A Library for Gaussian Processes and Variational Inference
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- Disentangling the Faraday rotation sky
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- Bayesian self-calibration and imaging in Very Long Baseline Interferometry
- Imaging a ring-like structure and the extended jet of M87 at 86 GHz
- A method for reconstructing the Galactic magnetic field using dispersion of fast radio bursts and Faraday rotation of radio galaxies
- Event-horizon-scale Imaging of M87* under Different Assumptions via Deep Generative Image Priors
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- DoG-HiT: A novel VLBI Multiscale Imaging Approach
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- Towards a Field Based Bayesian Evidence Inference from Nested Sampling Data