4.6 Article

CosmoDC2: A Synthetic Sky Catalog for Dark Energy Science with LSST

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出版社

IOP Publishing Ltd
DOI: 10.3847/1538-4365/ab510c

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资金

  1. US DOE [DE-AC02-06CH11357]
  2. Pittsburgh Particle Physics, Astrophysics and Cosmology Center through the Samuel P. Langley PITT PACC Postdoctoral Fellowship
  3. NASA through the NASA Hubble Fellowship - Space Telescope Science Institute [HST-HF2-51441.001]
  4. NASA [NAS5-26555]
  5. Centre National de la Recherche Scientifique
  6. National Energy Research Scientific Computing Center, a DOE Office of Science User Facility - Office of Science of the US Department of Energy [DE-AC02-05CH11231]
  7. STFC DiRAC HPC Facilities - UK BIS National E-infrastructure capital grants
  8. UK particle physics grid - GridPP Collaboration
  9. DOE [DE-AC02-76SF00515]
  10. DOE Office of Science User Facility [DE-AC02-06CH11357]
  11. National Science Foundation [PHY-1607611]
  12. W.M. Keck Foundation
  13. NSF [AST-95-09298, AST-0071048, AST-0507428, AST-0507483]
  14. NASA LTSA [NNG04GC89G]
  15. US Department of Energy Cosmic Frontier program [DE-SC0010118, DE-SC0010008]

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This paper introduces cosmoDC2, a large synthetic galaxy catalog designed to support precision dark energy science with the Large Synoptic Survey Telescope (LSST). CosmoDC2 is the starting point for the second data challenge (DC2) carried out by the LSST Dark Energy Science Collaboration (LSST DESC). The catalog is based on a trillion-particle, (4.225 Gpc)(3) box cosmological N-body simulation, the Outer Rim run. It covers 440 deg(2) of sky area to a redshift of z = 3 and matches expected number densities from contemporary surveys to a magnitude depth of 28 in the r band. Each galaxy is characterized by a multitude of galaxy properties including stellar mass, morphology, spectral energy distributions, broadband filter magnitudes, host halo information, and weak lensing shear. The size and complexity of cosmoDC2 requires an efficient catalog generation methodology; our approach is based on a new hybrid technique that combines data-based empirical approaches with semianalytic galaxy modeling. A wide range of observation-based validation tests has been implemented to ensure that cosmoDC2 enables the science goals of the planned LSST DESC DC2 analyses. This paper also represents the official release of the cosmoDC2 data set, including an efficient reader that facilitates interaction with the data.

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