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Mid-Range Science Objectives for the Event Horizon Telescope

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arxiv 2410.02986 v1 pith:GX3KDPZ5 submitted 2024-10-03 astro-ph.HE astro-ph.GA

classification astro-ph.HEastro-ph.GA
keywords blackdataopportunitiesrangeeventfirstholeshorizon
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The first images of the black holes in Sagittarius A* and M87* have created a wide range of new scientific opportunities in gravitational physics, compact objects, and relativistic astrophysics. We discuss here the scientific opportunities that arise from the rich data sets that have already been obtained and the new data sets that will be obtained, exploiting a wide range of technical advances, including observational agility, receiver upgrades, and the addition of new stations. This document provides a 5-year framework for Event Horizon Telescope (EHT) science structured around four fundamental questions that are used to prioritize the analysis of existing data, guide technical upgrades, and determine the optimal use of future observational opportunities with EHT, ALMA, and multi-wavelength facilities. Through enhancements over this period, the EHT will create the first movie of M87* connecting black hole and jet physics, provide detailed studies of the structure and dynamics of Sgr A*, characterize the magnetospheres of both systems through polarimetric imaging, and explore the spacetime properties of black holes with greater precision and range.

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Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Survey of Radiative, Two-Temperature Magnetically Arrested Simulations of the Black Hole M87* I: Turbulent Electron Heating

    astro-ph.HE 2025-01 conditional novelty 6.0 of 10

    Radiative two-temperature MAD simulations of M87* with Kawazura et al. (2019) turbulent electron heating match EHT total intensity but over-predict beam-scale linear polarization (about 30% versus the observed under 1...

  2. HST Observations within the Sphere of Influence of the Powerful Supermassive Black Hole in PKS0745-191

    astro-ph.GA 2025-01 conditional novelty 6.0 of 10

    Ionized gas within roughly 600 pc of the supermassive black hole in PKS 0745-191 is chaotic and non-rotating, with a sharp central velocity dispersion that suggests a black hole of about 1.5e10 solar masses.

  3. Dynamics and geometry of the inner sub-parsec-scale jet in 3C 279 observed with the Event Horizon Telescope

    astro-ph.GA 2026-07 conditional novelty 5.0 of 10

    EHT 2021 images of 3C 279 reveal an intrinsic, sideways-elongated jet base whose components move at apparent speeds up to 10c, implying a sub-parsec bend toward the observer and viewing angles below one degree.

  4. Deep learning inference with the Event Horizon Telescope II. The Zingularity framework for Bayesian artificial neural networks

    astro-ph.IM 2025-06 conditional novelty 5.0 of 10

    Bayesian neural networks trained on synthetic EHT observations of Sgr A* and M87* recover spin and magnetic state well in cross-code tests, but give overconfident wrong estimates for temperature ratio and inclination ...

  5. Characteristic precessions of spherical orbit around a rotating braneworld black hole

    gr-qc 2025-05 conditional novelty 5.0 of 10

    Positive tidal charge in rotating braneworld black holes suppresses nodal, periastron, and gyroscopic Lense-Thirring precession; negative tidal charge enhances them.

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