OpenUniverse2024: A shared, simulated view of the sky for the next generation of cosmological surveys

  • OpenUniverse
  • , The LSST Dark Energy Science Collaboration
  • , The Roman HLIS Project Infrastructure
  • , The Roman RAPID Project Infrastructure Team
  • , The Roman Supernova Cosmology Project Infrastructure Team
  • , A. Alarcon
  • , L. Aldoroty
  • , G. Beltz-Mohrmann
  • , A. Bera
  • , J. Blazek
  • , J. Bogart
  • , G. Braeunlich
  • , A. Broughton
  • , K. Cao
  • , J. Chiang
  • , N. E. Chisari
  • , V. Desai
  • , Y. Fang
  • , L. Galbany
  • , A. Hearin
  • K. Heitmann, C. Hirata, R. Hounsell, B. Jain, M. Jarvis, J. Jencson, A. Kannawadi, M. K. Kasliwal, R. Kessler, A. Kiessling, R. Knop, E. Kovacs, R. Laher, K. Laliotis, C. Lin, I. Lopes, E. Macbeth, A. Mahabal, R. Mandelbaum, J. Masiero, S. Mau, C. Meehan, J. Meyers, B. Moraes, R. Paladini, A. Pearl, A. Plazas Malagon, B. Rose, D. Rubin, B. Rusholme, A. Santos, N. Šarčević, D. Scolnic, J. Singhal, M. A. Troxel*
*Corresponding author for this work

Research output: Contribution to journalArticleAcademicpeer-review

Abstract

The OpenUniverse2024 simulation suite is a cross-collaboration effort to produce matched simulated imaging for multiple surveys as they would observe a common simulated sky. Both the simulated data and associated tools used to produce it are intended to uniquely enable a wide range of studies to maximize the science potential of the next generation of cosmological surveys. We have produced simulated imaging for approximately 70 deg of the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) Wide-Fast-Deep survey and the Nancy Grace Roman Space Telescope High-Latitude Wide-Area Survey, as well as overlapping versions of the ELAIS-S1 Deep-Drilling Field for LSST and the High-Latitude Time-Domain Survey for Roman. OpenUniverse2024 includes (i) an early version of the updated extragalactic model called Diffsky, which substantially improves the realism of optical and infrared photometry of objects, compared to previous versions of these models; (ii) updated transient models that extend through the wavelength range probed by Roman and Rubin; and (iii) improved survey, telescope, and instrument realism based on up-to-date survey plans and known properties of the instruments. It is built on a new and updated suite of simulation tools that improves the ease of consistently simulating multiple observatories viewing the same sky. The approximately 400 TB of synthetic survey imaging and simulated universe catalogs are publicly available, and we preview some scientific uses of the simulations.

Original languageEnglish
Pages (from-to)3799-3823
Number of pages25
JournalMonthly Notices of the Royal Astronomical Society
Volume544
Issue number4
DOIs
Publication statusPublished - 1 Dec 2025

Bibliographical note

Publisher Copyright:
© 2025 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.

Keywords

  • large-scale structure of Universe
  • software: simulations
  • transients: supernovae

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  • OpenUniverse2024: A shared, simulated view of the sky for the next generation of cosmological surveys

    OpenUniverse, OpenUniverse, The LSST Dark Energy Science Collaboration, The Roman HLIS Project Infrastructure Team, The Roman RAPID Project Infrastructure Team, The Roman Supernova Cosmology Project Infrastructure Team, Alarcon, A., Aldoroty, L., Beltz-Mohrmann, G., Bera, A., Blazek, J., Bogart, J., Braeunlich, G., Broughton, A., Cao, K., Chiang, J., Chisari, N. E., Desai, V., Fang, Y. & Galbany, L. & 31 others, Hearin, A., Heitmann, K., Hirata, C., Hounsell, R., Jain, B., Jencson, J., Kannawadi, A., Kasliwal, M. K., Kessler, R., Kiessling, A., Knop, R., Kovacs, E., Laher, R., Laliotis, K., Lopes, I., Mahabal, A., Mandelbaum, R., Masiero, J., Mau, S., Meehan, C., Meyers, J., Moraes, B., Paladini, R., Pearl, A., Plazas Malagon, A., Rose, B., Rusholme, B., Santos, A., Šarčević, N., Scolnic, D. & Troxel, M. A., 10 Jan 2025, arXiv, 25 p.

    Research output: Working paperPreprintAcademic

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