OpenUniverse 2024 Simulated Roman & Rubin Images: Preview

Overview

OpenUniverse2024 is a project to simulate spatially overlapping imaging surveys to be carried out by the Nancy Grace Roman Telescope and the Vera C. Rubin Observatory. The simulations were carried out on Argonne's Theta cluster and consist of:

  1. The LSST ELAIS-S1 Deep Drilling Field (DDF)
  2. The Roman Time-Domain Survey (TDS) shifted to overlap the ELAIS region and LSST DDF
  3. Overlapping LSST Wide-Fast-Deep (WFD) survey (with rolling cadence)
  4. Overlapping Roman Wide-Area Survey (WAS) in the same region
  5. A deep-field calibration region of the Roman WAS in the same region

This data preview release consists of a subset of data from each of the five categories above.

If you use OpenUniverse 2024 Preview data, please cite the dataset Digital Object Identifier (DOI): 10.26131/IRSA569. If you used the cloud-hosted copy of the data, also include the "How to Cite" text listed on the OpenUniverse2024 AWS Open Data Registry page.

Jump to documentation.

Data Set Characteristics

Data ProductDescriptionData Access
Images and Tables Roman & Rubin simulated images (FITS) and tables (Parquet)

These data are available on premises at IPAC and in the cloud via Amazon Web Services (AWS).

Bucket name: nasa-irsa-simulations
Bucket region: us-east-1

AWS Open Data Registry page: https://registry.opendata.aws/openuniverse2024/

  • S3 prefix for Roman simulated data: openuniverse2024/roman/preview/
  • S3 prefix for Rubin simulated data: openuniverse2024/rubin/preview/

On premises data access:

Project Team

  • Project Lead: Michael Troxel
  • OpenUniverse Team
  • Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) Dark Energy Science Collaboration (DESC)
  • Nancy Grace Roman Space Telescope Project Infrastructure Teams (PIT)
    • High-Latitude Imaging Survey (HLIS) PIT
    • Supernova (SN) PIT
    • Roman Alerts Promptly from Image Differencing (RAPID) PIT

Acknowledgements

This work was supported in part by the OpenUniverse effort, which is funded by NASA under JPL Contract Task 70-711320, "Maximizing Science Exploitation of Simulated Cosmological Survey Data Across Surveys". The DESC acknowledges ongoing support from the Institut National de Physique Nucléaire et de Physique des Particules in France; the Science & Technology Facilities Council in the United Kingdom; and the Department of Energy and the National Science Foundation in the United States. Work in the Roman HLIS PIT is supported by NASA grant 22-ROMAN11-0011, "Maximizing Cosmological Science with the Roman High Latitude Imaging Survey." Work in the Roman SN PIT is supported by NASA under award number 80NSSC24M0023, "A Roman PIT to Support Cosmological Measurements with Type Ia Supernovae". Argonne National Laboratory's work was supported under the U.S. Department of Energy contract DE-AC02-06CH11357. Work in the RAPID PIT is supported by NASA under the award number 80NSSC24M0020, "RAPID: Roman Alerts Promptly from Image Differencing". The SLAC National Accelerator Laboratory, operated under DOE Contract DE-AC02-76SF00515, is the host laboratory for DESC and manages support for the DESC pipeline scientist and computing infrastructure teams.

This research used resources of the Argonne Leadership Computing Facility, which is a DOE Office of Science User Facility supported under Contract DE-AC02-06CH11357. This work was done through a special ALCF Discretionary award using all of Theta before the system was retired. This research used resources of the National Energy Research Scientific Computing Center (NERSC), a Department of Energy Office of Science User Facility using NERSC award ERCAP0026324. This research used resources at the Duke Compute Cluster.

Additional Resources

Description of OpenUniverse 2024 data products
How to access IRSA-curated data sets in the cloud
Related Python Tutorials
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