Galaxies (Oct 2023)

Reference Array and Design Consideration for the Next-Generation Event Horizon Telescope

  • Sheperd S. Doeleman,
  • John Barrett,
  • Lindy Blackburn,
  • Katherine L. Bouman,
  • Avery E. Broderick,
  • Ryan Chaves,
  • Vincent L. Fish,
  • Garret Fitzpatrick,
  • Mark Freeman,
  • Antonio Fuentes,
  • José L. Gómez,
  • Kari Haworth,
  • Janice Houston,
  • Sara Issaoun,
  • Michael D. Johnson,
  • Mark Kettenis,
  • Laurent Loinard,
  • Neil Nagar,
  • Gopal Narayanan,
  • Aaron Oppenheimer,
  • Daniel C. M. Palumbo,
  • Nimesh Patel,
  • Dominic W. Pesce,
  • Alexander W. Raymond,
  • Freek Roelofs,
  • Ranjani Srinivasan,
  • Paul Tiede,
  • Jonathan Weintroub,
  • Maciek Wielgus

DOI
https://doi.org/10.3390/galaxies11050107
Journal volume & issue
Vol. 11, no. 5
p. 107

Abstract

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We describe the process to design, architect, and implement a transformative enhancement of the Event Horizon Telescope (EHT). This program—the next-generation Event Horizon Telescope (ngEHT)—will form a networked global array of radio dishes capable of making high-fidelity real-time movies of supermassive black holes (SMBH) and their emanating jets. This builds upon the EHT principally by deploying additional modest-diameter dishes to optimized geographic locations to enhance the current global mm/submm wavelength Very Long Baseline Interferometric (VLBI) array, which has, to date, utilized mostly pre-existing radio telescopes. The ngEHT program further focuses on observing at three frequencies simultaneously for increased sensitivity and Fourier spatial frequency coverage. Here, the concept, science goals, design considerations, station siting, and instrument prototyping are discussed, and a preliminary reference array to be implemented in phases is described.

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