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    • About
    • History
    • Who was Vera Rubin?
    • Construction Updates
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      • Rubin in Chile
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      • Leadership
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      • Work With Us
      • Jobs Board
    • Explore
      • How Rubin Works
      • Legacy Survey of Space and Time (LSST)
      • Rubin Technology
      • Alert Stream
      • Rubin Numbers
    • Science Goals
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      • Activities, Games, and More
      • Space Surveyors Game
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      • Animated Video Series
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    • For Media
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      • Resources for scientists
      • Rubin Community Forum
      • Early Science Program
      • Workshops and seminars
      • Tutorials
      • LSST Discovery Alliance
      • Code of Conduct
      • Survey, instruments, and telescopes
      • Key numbers
      • The Legacy Survey of Space and Time (LSST)
      • Instruments
      • Telescopes
      • Data products, pipelines, and services
      • Data access and analysis
      • Recent data releases
      • Alerts and brokers
      • Data processing pipelines
      • Future data products
      • Data Policy
      • Documentation and publications
      • Technical documentation
      • How to cite Rubin Observatory
      • Publication policies
      • Science Collaborations
      • Galaxies Science Collaboration
      • Stars, Milky Way, and Local Volume Science Collaboration
      • Solar System Science Collaboration
      • Dark Energy Science Collaboration
      • Active Galactic Nuclei Science Collaboration
      • Transients and Variable Stars Science Collaboration
      • Strong Lensing Science Collaboration
      • Informatics and Statistics Science Collaboration
    • Citizen Science
      • Committees and teams
      • Science Advisory Committee (SAC)
      • Survey Cadence Optimization Committee (SCOC)
      • Users Committee
      • Community Science Team (CST)
      • Research Inclusion Group
      • Project Science Team (PST)
    • Education
    • Education FAQs
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The U.S. National Science Foundation (NSF) and the U.S. Department of Energy (DOE) Office of Science will support Rubin Observatory in its operations phase to carry out the Legacy Survey of Space and Time. They will also provide support for scientific research with the data. During operations, NSF funding is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with NSF, and DOE funding is managed by SLAC National Accelerator Laboratory (SLAC), under contract by DOE. Rubin Observatory is operated by NSF NOIRLab and SLAC.

NSF is an independent federal agency created by Congress in 1950 to promote the progress of science. NSF supports basic research and people to create knowledge that transforms the future.

The DOE Office of Science is the single largest supporter of basic research in the physical sciences in the United States and is working to address some of the most pressing challenges of our time.

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  1. For Scientists
  2. Survey, instruments, and telescopes

Survey, instruments, and telescopes

Key Numbers

A quick reference for the telescope, site, camera, and survey.

LSST key numbers

Legacy Survey of Space and Time (LSST)

All data collected by the Rubin Observatory is part of the science-driven, community-optimized Legacy Survey of Space and Time (LSST).

The Legacy Survey of Space and Time (LSST)

Instruments

The LSST Science Camera is the world's largest digital camera, with 3.2 Gigapixels and six filters.

The LSST Science Camera and the Commissioning Camera.

Telescopes

The main Simonyi Survey Telescope and the nearby Auxiliary Telescope (AuxTel) for calibrations.

The Simonyi Survey Telescope and AuxTel.

Site

Located atop Cerro Pachón in Chile, next to the Gemini South and SOAR Observatories, with a latitude and longitude of 30º14'40.68"S, 70º44'57.90"W and an elevation of 2647 meters.

The observatory facility page (for a public audience).