Published July 22, 2024 | Published
Conference Paper Open

Innovations and advances in instrumentation at the W. M. Keck Observatory, vol. III

Kassis, Marc F.1
Alvarez, Carlos1
Baker, Ashley D.2 ORCID icon
Bailey, John I.2
Banyal, Ravinder K.3 ORCID icon
Bertz, Rob2
Beichman, Charles A.4 ORCID icon
Bouchez, Antonin H.1 ORCID icon
Brown, Aaron M.5
Brown, Matthew K.1
Bundy, Kevin A.6
Campbell, Randall D.1
Chun, Mark R.7
Cooke, Jeffrey8
Deich, William T.9
Dekany, Richard G.2 ORCID icon
Doppmann, Greg1
Fassnacht, Christopher10
Ferrara, Jocelyn2
Fitzgerald, Michael P.11
Fremling, Christoffer2 ORCID icon
Fucik, Jason R.2
Gibson, Steven R.2
Gillingham, Peter R.12
Glazebrook, Karl8
Greffe, Timothee2 ORCID icon
Halverson, Samuel P.2
Hill, Grant M.1
Hillenbrand, Lynne A.2
Hinz, Philip M.9
Holden, Bradford P.9 ORCID icon
Howard, Andrew W.2 ORCID icon
Huber, Daniel7
Jones, Tucker A.10
Jordan, Carolyn1
Jovanovic, Nemanja J.2 ORCID icon
Kain, Isabel J.6
Kasliwal, Mansi M.2 ORCID icon
Kirby, Evan13
Konopacky, Quinn M.5 ORCID icon
Krishnan, Shanti8
Kulkarni, Shrinivas R.2 ORCID icon
Kupke, Renate9 ORCID icon
Lanclos, Kyle1 ORCID icon
Larkin, James E.11
Lilley, Scott J.1
Lingvay, Larry2
Lu, Jessica R.14 ORCID icon
Lyke, James E.1
MacDonald, Nicholas9
Martin, Christopher2 ORCID icon
Mather, John C.15
Matuszewski, Mateusz2
Mawet, Dimitri2 ORCID icon
McGurk, Rosalie C.1 ORCID icon
Marin, Eduardo1 ORCID icon
Meeks, Robert L.1
Millar-Blanchaer, Maxwell A.16 ORCID icon
Nash, Reston B.2
Neill, James D.2
O'Meara, John M.1 ORCID icon
Pahuja, Rishi2
Peretz, Eliad15
Prusinski, Nikolaus2 ORCID icon
Radovan, Matthew V.2
Rider, Kodi A.17
Roberts, Mitsuko K.2
Rockosi, Constance M.6
Rubenzahl, Ryan2 ORCID icon
Sallum, Stephanie E.18
Sandford, Dale9
Savage, Maureen L.9
Skemer, Andrew J.6
Smith, Roger2
Steidel, Charles C.2 ORCID icon
Steiner, Jonathan1
Stelter, Richard D.9 ORCID icon
Walawender, Josh1 ORCID icon
Westfall, Kyle B.9 ORCID icon
Wizinowich, Peter L.1 ORCID icon
Wright, Shelley A.5
Wold, Truman1
Zimmer, Jake2
  • 1. ROR icon W.M. Keck Observatory
  • 2. ROR icon California Institute of Technology
  • 3. Indian Institute of Astronomy (India)
  • 4. ROR icon NASA Exoplanet Science Institute
  • 5. ROR icon University of California, San Diego
  • 6. ROR icon University of California, Santa Cruz
  • 7. ROR icon University of Hawaii System
  • 8. ROR icon Swinburne University of Technology
  • 9. Univ. of California Observatories (United States)
  • 10. ROR icon University of California, Davis
  • 11. ROR icon University of California, Los Angeles
  • 12. ROR icon Macquarie University
  • 13. ROR icon University of Notre Dame
  • 14. ROR icon University of California, Berkeley
  • 15. ROR icon Goddard Space Flight Center
  • 16. ROR icon University of California, Santa Barbara
  • 17. Univ. of California (United States)
  • 18. ROR icon University of California, Irvine

Abstract

Since the start of science operations in 1993, the twin 10-meter W. M. Keck Observatory (WMKO) telescopes have continued to maximize their scientific impact to produce transformative discoveries that keep the U.S. observing community on the frontiers of astronomical research. Upgraded capabilities and new instrumentation are provided though collaborative partnerships primarily with the Caltech and University of California instrument development teams and through additional collaborations with the University of Notre Dame, the University of Hawaii, Swinburne University of Technology, industry, and other organizations. This paper summarizes the status and performance of observatory infrastructure projects, technology upgrades, and new additions to the suite of observatory instrumentation. We also provide a status of instrumentation projects in early and advanced stages of development that will achieve the goals and objectives summarized in the 2023 Keck Observatory strategic plan. Developed in collaboration with the WMKO science community, the Keck strategic plan sets our sites on 2035 and meets goals identified in the Astro2020 Decadal Survey.

Copyright and License

© (2024) Society of Photo-Optical Instrumentation Engineers (SPIE).

Acknowledgement

KPF was supported by the National Science Foundation under Grant # 2034278, by the Heising-Simons Foundation with grants 2016-042, 2018-0905, & a loan, as well as the Mt. Cuba Astronomical Foundation. KCRM is supported in part by the National Science Foundation under Grant No. AST-1429890. KAPA is supported in part by the National Science Foundation under grant No. AST-1836016. SCALES is supported by the Heising-Simons Foundation, Mt. Cuba Astronomical Foundation, and the National Science foundation under grant No. AST-2216481. Liger is partially supported by the Heising-Simons Foundation, Gordon and Betty Moore Foundation, and by the National Science Foundation under grant No. AST-2308190. HISPEC is supported by the Caltech fund for Keck instrumentation, the Gordon and Betty Moore Foundation, the Heising-Simon Foundation and has benefitted from in-kind contributions from NASA, the AstroBiology Center (NINS), Northwestern, and the University of Toronto. LRIS-2 is supported by the Caltech fund for Keck instrumentation.

Some of the data presented herein were obtained at Keck Observatory, which is a private 501(c)3 non-profit organization operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation.

This research was carried out, in part, at the Jet Propulsion Laboratory and the California Institute of Technology under a contract with the National Aeronautics and Space Administration and funded through the President’s and Director’s Research\& Development Fund Program.

The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Maunakea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain.

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Additional details

Created:
April 8, 2025
Modified:
April 8, 2025