Localize site content
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
      • How Rubin Works
      • Legacy Survey of Space and Time (LSST)
      • Rubin Technology
      • Alert Stream
      • Rubin Numbers
    • Science Goals
      • Skyviewer ↗
      • Skysynth: The cosmos captured by Rubin, for your ears
    • Orbitviewer ↗
    • Rubin Voices
    • 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
    • Slideshows
    • Construction Archive Gallery
    • Media Use Policy
    • News
    • Press Releases
      • Rubin Observatory First Look
      • The Cosmic Treasure Chest
      • A Swarm of New Asteroids
      • Rhythms in the Stars
      • Trifid and Lagoon Nebulae
      • Rubin First Look Watch Parties
    • 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
      • LSST Discovery Alliance
      • Public outreach materials
      • For amateur astronomers
      • Survey, instruments, and telescopes
      • Key numbers
      • 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
      • Resources
      • In-Kind Program FAQs
      • Frequently Asked Questions
      • 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
  • 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

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 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
    • 2021_0312_LSST_R_Filter_Lange-46.jpg
    • The tiled blue focal plane of the LSST Camera, viewed nearly edge on and from slightly below. The focal plane is made of 189 CCD chips arranged in a roughly square shape with its corners cut off. The focal plane is set within a shiny metal ring, which the other components of the camera will be attached to.
      Vera C. Rubin Observatory LSST Camera Focal Plane
    • Two pairs of human legs extend from beneath the suspended system, which has a golden, cylindrical housing
      Filter exchange
    • The glass lens of the huge LSST Camera inside its black carbon fiber casing. The curvature of the lens extends above the rim of the black casing, like a glass of water about to overflow. Four people in white head-to-toe clean room suits stand in a circle in the background of this white room.
      The LSST Camera Lens is here!
    • A person in a full head-to-toe white clean room suit works beneath one of the LSST Camera CCD rafts suspended from a metal support. The CCD raft contains nine CCD chips arranged in a square. The chips are oriented to face the work space below. The image is focused on the CCD raft, and the person standing behind is slightly blurred and out of focus.
      LSST 1st Science Raft
    • Secondary Mirror (M2) coating in 2019
    • Timelapse of secondary mirror coating
    • a worker uses a magnifying headset to work on exposed circuitry of the filter changer
      Working on the autochanger
    • A top down view looking at the incomplete LSST Camera focal plane. At the center is a tiled metal frame that looks like a 4 by 4 checkerboard, with empty squares. The lines making up the checkered pattern are a light copper color and run diagonally from upper left to lower right, and from lower left to upper right. The checkered pattern is inside a metal cylinder structure with various metal pipes around the outside. All of the metal is extremely clean and shiny.
      Vera C. Rubin Observatory LSST Camera Focal Plane Build
    • M2 testing
    • M2 testing
    • Precision Optics Group at Harris
    Showing 151 to 175 of 175
    • 1
    • 2
    • 3
    • 4
    • 5
    • 6
    Previous  Next
    <<
    >>
    Galleries
    • Main Gallery
    • Featured Media
    • News Gallery
    • First Look
    • Graphics & Illustrations
    • Outreach & Education