REVIEW article

Front. Astron. Space Sci.

Sec. Astronomical Instrumentation

Volume 12 - 2025 | doi: 10.3389/fspas.2025.1608411

Nearly a Decade of Groundbreaking Speckle Interferometry at the International Gemini Observatory

Provisionally accepted
Steve  B HowellSteve B Howell1*Clara  Martinez-VazquezClara Martinez-Vazquez2Elise  FurlanElise Furlan3Nic  ScottNic Scott4Rachel  MatsonRachel Matson5Colin  LittlefieldColin Littlefield1,6Catherine  ClarkCatherine Clark3Katie  LesterKatie Lester7Zach  hartmanZach hartman1Davd  CiardiDavd Ciardi3Sarah  DevenySarah Deveny1,6
  • 1Ames Research Center, National Aeronautics and Space Administration, Moffet Field, United States
  • 2Gemini Observatory, Hawaiian Acres, Hawaii, United States
  • 3NASA Exoplanet Science Institute, California Institute of Technology, Pasadena, California, United States
  • 4Center for High Angular Resolution Astronomy, Georgia State University, Atlanta, Colorado, United States
  • 5United States Naval Observatory (USNO), Washington, District of Columbia, United States
  • 6Bay Area Environmental Research Institute, Moffett Field, United States
  • 7Mount Holyoke College, South Hadley, Massachusetts, United States

The final, formatted version of the article will be published soon.

Since its inception, speckle interferometry has revolutionized high-resolution astronomical imaging, overcoming atmospheric challenges to achieve the diffraction limits of telescopes.Almost a decade ago, in 2018, a pair of speckle cameras -'Alopeke and Zorro -were installed at two of the largest apertures in the world, the twin 8.1-meter Gemini North and South telescopes in Hawai'i and Chile. Equipped with dual blue and red channels, 'Alopeke and Zorro deliver high-resolution imaging across the optical bandpass from 350 to 1000 nm, which has led to crucial discoveries in both stellar multiplicity and exoplanetary science. Furthermore, the broad and nonrestrictive access to these instruments, given by each Gemini Observatory partner and via the US NOIRLab open skies policy, has allowed the community to expand the applications of the instruments, supporting a wide range of scientific investigations from Solar System bodies, to morphological studies of stellar remnants and quasars, to evolved stars, to transient phenomena. This paper reviews the instrument technology and observational capabilities, and highlights key scientific contributions and discoveries of 'Alopeke and Zorro, emphasizing the enduring importance of speckle interferometry in advancing modern observational astronomy and expanding the frontiers of astronomical research.

Keywords: binary stars, Planet Hosting Stars, Speckle interferometry, Astronomical Techniques, High angular resolution

Received: 08 Apr 2025; Accepted: 05 May 2025.

Copyright: © 2025 Howell, Martinez-Vazquez, Furlan, Scott, Matson, Littlefield, Clark, Lester, hartman, Ciardi and Deveny. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) or licensor are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.

* Correspondence: Steve B Howell, Ames Research Center, National Aeronautics and Space Administration, Moffet Field, United States

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