Homepage
Localize site content
    • 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: Skyviewer, sonfied
    • 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 COSMOS
      • 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
      • Data Policy
      • Data policy slides
      • News, events, and deadlines
      • Rubin Science Assemblies
      • Rubin Data Academy
      • Rubin Community Workshop
      • Resources for scientists
      • Rubin Community Forum
      • Early Science Program
      • LSST Discovery Alliance
      • Workshops and seminars
      • Tutorials
      • Additional compute resources
      • Gemini time for alert follow-up
      • 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 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
  • 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

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
    1. For Scientists
    2. Committees and teams
    3. Users Committee

    Users Committee

    Date last updated: 30 Oct 2026 10:32 (MST)

    About: The Rubin Users Committee (UC) is charged with assessing the scientific utility of the Rubin data products and Science Platform, and reporting their findings in twice-yearly reports to the Rubin Operations director. UC charge document.

    Meetings and reports: Meetings of the UC begin with a 'listening session', and all members of the Rubin community are welcome to attend and raise issues for UC discussion. A meeting calendar is posted below. Meeting announcements, connection info, and the twice-yearly reports are available in the Rubin Community Forum as topics with the users-committee tag.

    Contact: The UC encourages feedback from the Rubin community, and can be contacted via direct message to the @Users-Committee group in the Rubin Community Forum or by email to RubinObs-Users-Committee@lists.lsst.org.

    Current Members

    Chair: Vincenzo Petrecca

    James Freeburn (he/him) is a Postdoctoral researcher at the University of North Carolina at Chapel Hill. He works in time domain astronomy, primarily on identification and multi-wavelength follow-up of fast optical transients including GRB afterglows and kilonovae. He is a member of Rubin's Transients and Variable Stars collaboration.

    Sugata Kaviraj () - TBD

    Fatoumata Kebe () - TBD

    Mike Kelley (he/him) - Principal Research Scientist at the University of Maryland, College Park. He studies small solar system objects, especially cometary activity, outbursts, surfaces, and dust properties. He is a member of the Solar System Science Collaboration.

    Surhud More () - TBD

    Alejandra Muñoz Arancibia (she/her) – ALeRCE Data Scientist at the Millennium Institute of Astrophysics (MAS), hosted at the Center for Mathematical Modeling (CMM), Chile. Experience in cosmological simulations of galaxy formation and evolution, models and observations of dusty star-forming galaxies, and data analysis of transients and variables in general. Member of the ALeRCE alert broker, DESC, and ISSC.

    Ryan Oelkers (he/him) - Assistant Professor at the University of Texas Rio Grande Valley. His research focuses on exoplanet detection and demographics, ground-based instrumentation, and the analysis of large-scale photometric data. Prior to joining the faculty at UTRGV, he spent two years in industry as a data scientist, and he was member of the targeting teams for TESS and APOGEE-2N.

    Vincenzo Petrecca (he/him) – Postdoctoral researcher at INAF-Observatory of Capodimonte, Italy. His research focuses on time domain astronomy, particularly on AGN optical variability and Supernovae. Experience in time series analysis (both in time and frequency domain), photometric classification, and rate measurements of transient sources. He is a member of DESC, TVS and AGN Science Collaborations.

    Elham Saremi (she/her) is a Research Fellow at the University of Southampton, UK, working on the development of the LSST–VISTA Fusion pipeline. Her work focuses on integrating near-infrared observations from VISTA with optical data from the Vera C. Rubin Observatory, enabling combined multiwavelength imaging and catalogues for scientific analysis. Her research interests include galaxy evolution, with a particular focus on low-surface-brightness structures, dwarf galaxies, and faint galaxy outskirts in the near-infrared. She is a member of three Rubin LSST Science Collaborations: Galaxies; Active Galactic Nuclei (AGN); and Stars, Milky Way, and Local Volume.

    Argyro Sasli (she/her) – Research Scientist at the University of Minnesota, School of Physics and Astronomy, USA. Her research spans time-domain astronomy, gravitational-wave astrophysics, and machine learning, with experience in multimodal transient classification, anomaly detection, alert brokering, and uncertainty quantification for large surveys. She is lead developer of the AppleCiDEr multimodal transient classifier, chairs the ZTF machine learning subgroup, and co-chairs the real-real classification group of Roman STRIDE.

    Darryl Seligman (he/him) – Assistant Professor at Michigan State University Department of Physics and Astronomy. Experience in small bodies in the Solar System including interstellar objects and dark comets, nonlinear dynamics, MHD and fluid dynamics.

    Charlotte Ward (she/her) - Assistant Professor at the Pennsylvania State University with a science focus on AGN, tidal disruption events, and lensed supernovae and technical interests in joint pixel analysis of Rubin and overlapping space-based surveys. Member of DESC and the AGN SC.

    Michael Wood-Vasey (he/him) – Professor at the University of Pittsburgh. Science focus on supernova cosmology. Technical interests in large-survey image processing, image subtraction, and data-intensive astronomical analysis. Member of DESC and TVS.

    Past members

    Igor Andreoni, Dominique Boutigny, Matthew Holman, Anupreeta More, Vicki Sarajedini, Anja von der Linden, Matthew P. Wiesner, Alessandra Corsi, Francisco Javier Sanchez Lopez, Markus Rabus, Qingling Ni, V. Ashley Villar

    Meetings

    Meetings of the Users Committee begin with a 'listening session', and all members of the Rubin community are welcome to attend and raise issues for UC discussion.

    Slides

    These slides are kept up-to-date and made available to be linked into other slide decks.

    Go the slide decks with UC member names and faces, and UC information.