Localize site content
  • Contact Us
  • Jobs Board
  • Intranet
  • Visual Identity Guide
  • Privacy Policy

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.

Funding agency logos
Homepage
    • About
    • History
    • Who was Vera Rubin?
      • Rubin in Chile
      • Cerro Pachón
      • Observatory Site Selection
      • Organization
      • Leadership
      • Science Collaborations
    • Funding Information
      • Work With Us
      • Jobs Board
    • Explore
    • Rubin Basics
    • Science Goals
      • How Rubin Works
      • Legacy Survey of Space and Time (LSST)
      • Rubin Technology
      • Alert Stream
      • Rubin Numbers
    • Rubin Voices
      • Skyviewer ↗
      • Skysynth: The cosmos captured by Rubin, for your ears
    • Orbitviewer ↗
    • Get Involved in Rubin Research
      • Activities, Games, and More
      • Space Surveyors Game
      • Animated Video Series
    • Gallery
      • Main Gallery
      • Featured Media
      • News Gallery
      • First Look
      • Graphics & Illustrations
      • Outreach & Education
      • Image Releases
      • Rubin's Ocean of Stars
      • Rubin Observatory First Look
    • Slideshows
    • Construction Archive Gallery
    • Media Use Policy
    • News
    • Press Releases
    • Media Resources
    • Press Releases
    • Name Guidelines
    • For Scientists
    • Get started
      • News, events, and deadlines
      • Rubin Science Assemblies
      • Rubin Data Academy
      • Rubin Community Workshop
      • Resources for scientists
      • Rubin Community Forum
      • Early Science Program
      • Workshops and seminars
      • Tutorials
      • Additional compute resources
      • Gemini time for alert follow-up
      • LSST Discovery Alliance
      • Public outreach materials
      • For amateur astronomers
      • Survey, instruments, and telescopes
      • Key numbers
      • Live status
      • The Legacy Survey of Space and Time (LSST)
      • Instruments
      • Telescopes
      • Data products, pipelines, and services
      • Data Policy
      • Data access and analysis
      • Recent data releases
      • Alerts and brokers
      • Data processing pipelines
      • User-contributed resources
      • Future data products
      • Simulation software
      • Documentation and publications
      • Technical documentation
      • How to cite Rubin Observatory
      • Publication policies
      • Glossary & Acronyms
      • Papers citing Rubin Observatory
      • 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
      • Target of Opportunity (ToO) Advisory Board
      • Resource Allocation Committee (RAC)
      • Community Science Team (CST)
      • Research Inclusion Working Group (RIWG)
      • Project Science Team (PST)
      • In Kind Program
      • In-Kind Program FAQs
      • Frequently Asked Questions
      • Impacts from artificial satellites and debris
      • How to navigate this website
      • Code of Conduct
      • Interim CoC
    • Education
    • First Look Resources for Lasting Impact
    • Education FAQs
    • Educators
    • Glossary
    • Investigations
    • Calendar
Localize site content

News Gallery

Showing 151 to 0 of 0
  • 1
Previous  Next
<<
>>

Let's Connect

  • Visit the Rubin Observatory on Facebook
  • Visit the Rubin Observatory on Instagram
  • Visit the Rubin Observatory on LinkedIn
  • Visit the Rubin Observatory on Twitter
  • Visit the Rubin Observatory on YouTube
    • LSST Camera moves out of the clean room at SLAC
    • SLAC Family Day 2024
    • The LSST Camera, the largest camera ever built for astronomy. The camera opening is a large black ring with glass lenses, a bit smaller than a person is tall. In the center of the opening is the camera's focal plane detector, which is made of 189 square CCD chips arranged in a roughly square shape. The camera is suspended on a white metal frame with white handrails. The completely white room gives the image an overall sterile feel.
      LSST Camera at SLAC
    • The LSST Camera, the largest camera ever built for astronomy. The camera opening is a large black ring with glass lenses, a bit smaller than a person is tall. In the center of the opening is the camera's focal plane detector, which is made of 189 square CCD chips arranged in a roughly square shape. The camera is suspended on a white metal frame with white handrails. The completely white room gives the image an overall sterile feel.
      LSST Camera at SLAC
    • The lens of the LSST Camera, the largest camera ever built for astronomy, viewed from the side. The camera opening at right is a large black ring with glass lens bulging out, a bit smaller than a person is tall. Two people in white clean room suits at left pull a giant lens cover that's suspended off the ground toward the lens. The completely white room gives the image an overall sterile feel.
      LSST Camera at SLAC
    • Two large hauling trucks pull a 28-foot-wide, white hexagon-shaped box on a flat trailer up a grated dirt desert road. The white hexagonal box holds Rubin Observatory’s 8.4-meter combined  primary/tertiary glass mirror.
      M1M3 glass move March 7, 2024Rubin’s 8.4-meter Mirror Moves into the Observatory
    • Camera Filter Team
    • 2024_0222_LSST_IN2P3_Bonin_SLAC-15.jpg
    • LSST camera and SLAC camera team
    • LSST camera and SLAC camera team
    • LSST camera at SLAC
    • LSST camera and SLAC camera team
    • LSST camera at SLAC
    • LSST camera and SLAC camera team
    • LSST camera and SLAC camera team
    • LSST camera and SLAC camera team
    • Completed LSST Camera
    • LSST camera at SLAC
    • LSST camera and SLAC camera team
    • Rubin Observatory stands prominently in the center of this image atop its Chilean desert summit on Cerro Pachón. The sky is clear blue, and the setting sun glows from the left, illuminating the left side of the observatory. A large crane sits to the right of the observatory with its arm extended, looking small compared to the observatory building. The foreground summit area is shadowed, and the desert mountains recede into the distance, interspersed with hazy atmosphere. The telescopes of the neighboring Cerro Tololo Inter-American Observatory are visible as tiny bumps on a distant summit to the right.
      Rubin Sunset December 2023
    • Cleaning and testing Rubin's secondary mirror, March 2023
    • A view looking into the LSST Camera's huge opening. The camera opening is a large black donut shape, with reflections of ceiling light revealing the presence of glass lenses. In the center of the opening is the camera's focal plane detector, which is made of 189 square CCD chips arranged in a roughly square shape. The camera is suspended on a white metal frame with white handrails. The completely white room gives the image an overall sterile feel.
      Face to Face with the LSST Camera
    • A group of six people stand in front of the huge LSST digital camera, which is oriented so that we're looking into the lens opening and at the blue-tinted tiled focal plane of CCDs. The group of people are all outfitted head to toe in white clean room garb, with hair caps, face masks, white onesies, and foot covers.
      Lens cap off
    • A large gold metal ring surrounds the LSST Camera focal plane
      Camera entrance lens
    • LSST Cryostat to Camera Body Lift-135
    • A view looking through the L1 lens, showing a person inspecting it from behind. The lens is taller than the person.
      L1 lens for the LSST Camera
    • 3 persons in clean room suits work on the outer ring of the elevated L3 lens. The raft of camera sensors is visible through the lens.
      L3 Installation
    • 4 of the LSST camera filters are stored in a portable glass enclosure
      Four camera filters finished
    • Vera C. Rubin.jpeg
    • romanesco.png
    Showing 151 to 180 of 192
    • 1
    • 2
    • 3
    • 4
    • 5
    • 6
    • 7
    Previous  Next
    <<
    >>
    Galleries
    • Main Gallery
    • Featured Media
    • News Gallery
    • First Look
    • Graphics & Illustrations
    • Outreach & Education
    • Wildlife of Cerro Pachón