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A Joint Roman Space Telescope and Rubin Observatory Synthetic Wide-Field Imaging Survey

Journal Article · · Monthly Notices of the Royal Astronomical Society

We present and validate 20 deg(2) of overlapping synthetic imaging surveys representing the full depth of the Nancy Grace Roman Space Telescope High-Latitude Imaging Survey (HLIS) and 5 yr of observations of the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST). The two synthetic surveys are summarized, with reference to the existing 300 deg(2) of LSST simulated imaging produced as part of Dark Energy Science Collaboration (DESC) Data Challenge 2 (DC2). Both synthetic surveys observe the same simulated DESC DC2 universe. For the synthetic Roman survey, we simulate for the first time fully chromatic images along with the detailed physics of the Sensor Chip Assemblies derived from lab measurements using the flight detectors. The simulated imaging and resulting pixel-level measurements of photometric properties of objects span a wavelength range of similar to 0.3-2.0 mu m. We also describe updates to the Roman simulation pipeline, changes in how astrophysical objects are simulated relative to the original DC2 simulations, and the resulting simulated Roman data products. We use these simulations to explore the relative fraction of unrecognized blends in LSST images, finding that 20-30 per cent of objects identified in LSST images with i-band magnitudes brighter than 25 can be identified as multiple objects in Roman images. These simulations provide a unique testing ground for the development and validation of joint pixel-level analysis techniques of ground- and space-based imaging data sets in the second half of the 2020s - in particular the case of joint Roman-LSST analyses.

Research Organization:
Argonne National Laboratory (ANL), Argonne, IL (United States)
Sponsoring Organization:
United Kingdom Science and Technology Facilities Council; Centre National de la Recherche Scientifique (CNRS); National Science Foundation (NSF); National Aeronautics and Space Administration (NASA); USDOE Office of Science (SC)
DOE Contract Number:
AC02-06CH11357
OSTI ID:
2212479
Journal Information:
Monthly Notices of the Royal Astronomical Society, Vol. 522, Issue 2
Country of Publication:
United States
Language:
English

References (63)

A Method for Optimal Image Subtraction August 1998
Optimizing LSST observing strategy for weak lensing systematics September 2020
The brighter-fatter effect and pixel correlations in CCD sensors March 2014
Deblending galaxies with variational autoencoders: A joint multiband, multi-instrument approach October 2020
Testing lsst Dither Strategies for Survey Uniformity and Large-Scale Structure Systematics September 2016
SEP: Source Extractor as a library October 2016
Galacticus: A semi-analytic model of galaxy formation February 2012
SExtractor: Software for source extraction June 1996
Optimization of the Observing Cadence for the Rubin Observatory Legacy Survey of Space and Time: A Pioneering Process of Community-focused Experimental Design December 2021
Brighter-fatter Effect in Near-infrared Detectors. II. Autocorrelation Analysis of H4RG-10 Flats December 2019
An end-to-end simulation framework for the Large Synoptic Survey Telescope August 2014
The Ellipticity Distribution of Ambiguously Blended Objects December 2015
The LSST Scheduler from design to construction July 2016
The LSST operations simulator August 2014
Cosmology with the Roman Space Telescope : synergies with the Rubin Observatory Legacy Survey of Space and Time March 2021
2D-FFTLog: efficient computation of real-space covariance matrices for galaxy clustering and weak lensing June 2020
Beyond Limber: efficient computation of angular power spectra for galaxy clustering and weak lensing May 2020
Brighter-fatter Effect in Near-infrared Detectors—III. Fourier-domain Treatment of Flat Field Correlations and Application to WFIRST June 2020
Drizzle: A Method for the Linear Reconstruction of Undersampled Images February 2002
Quantum Yield and Charge Diffusion in the Nancy Grace Roman Space Telescope Infrared Detectors January 2022
Photometric Redshifts with the LSST. II. The Impact of Near-infrared and Near-ultraviolet Photometry May 2020
dustmaps: A Python interface for maps of interstellar dust June 2018
Candels: the Cosmic Assembly Near-Infrared deep Extragalactic Legacy Survey December 2011
Characterization and correction of charge-induced pixel shifts in DECam May 2015
Evidence for self-interaction of charge distribution in charge-coupled devices February 2015
Generating synthetic cosmological data with GalSampler June 2020
The Outer Rim Simulation: A Path to Many-core Supercomputers November 2019
Brighter-fatter Effect in Near-infrared Detectors. I. Theory of Flat Autocorrelations December 2019
Matplotlib: A 2D Graphics Environment January 2007
LSST: From Science Drivers to Reference Design and Anticipated Data Products March 2019
CCD Charge Collection Efficiency And The Photon Transfer Technique December 1985
The skewness of the aperture mass statistic July 2004
The Milky Way Tomography with SDSS. I. Stellar Number Density Distribution February 2008
The Impact of Interpixel Capacitance in CMOS Detectors on PSF Shapes and Implications for WFIRST June 2016
CANDELS: THE COSMIC ASSEMBLY NEAR-INFRARED DEEP EXTRAGALACTIC LEGACY SURVEY—THE HUBBLE SPACE TELESCOPE OBSERVATIONS, IMAGING DATA PRODUCTS, AND MOSAICS December 2011
CosmoDC2: A Synthetic Sky Catalog for Dark Energy Science with LSST December 2019
Validating Synthetic Galaxy Catalogs for Dark Energy Science in the LSST Era January 2022
cosmolike – cosmological likelihood analyses for photometric galaxy surveys May 2017
Radiation-induced Backgrounds in Astronomical Instruments: Considerations for Geosynchronous Orbit and Implications for the Design of theWFIRSTWide-field Instrument February 2016
Poisson_CCD: A dedicated simulator for modeling CCDs October 2021
Combining Undersampled Dithered Images February 1999
Impact of image persistence in the Roman Space Telescope High-Latitude Survey February 2022
The ACADIA ASIC - detector control and digitization for the Wide-Field Infrared Survey Telescope (WFIRST) July 2018
The LSST DESC DC2 Simulated Sky Survey March 2021
The SAGA Survey. II. Building a Statistical Sample of Satellite Systems around Milky Way–like Galaxies February 2021
The challenge of blending in large sky surveys August 2021
Evaluations Of Charge-Coupled Device (CCD) Performance For Astronomical Use January 1981
Properties and characteristics of the Nancy Grace Roman Space Telescope H4RG-10 detectors October 2020
A Framework for Telescope Schedulers: With Applications to the Large Synoptic Survey Telescope March 2019
Galaxy blending effects in deep imaging cosmic shear probes of cosmology May 2022
An Improved Photometric Calibration of the Sloan Digital Sky Survey Imaging Data February 2008
The Effect of Detector Nonlinearity on WFIRST PSF Profiles for Weak Gravitational Lensing Measurements September 2016
Hot pixel behavior in WFC3 CCD detectors irradiated under operational conditions January 2004
Simple improved reference subtraction for H4RG, H2RG, and H1RG near-infrared array detectors April 2022
Scientific Synergy between LSST and Euclid December 2017
GalSim: The modular galaxy image simulation toolkit April 2015
Effects of overlapping sources on cosmic shear estimation: Statistical sensitivity and pixel-noise bias July 2021
Photometric Calibration of the First 1.5 Years of the Pan-Starrs1 Survey August 2012
Mapping electrical crosstalk in pixelated sensor arrays August 2008
A theory for image persistence in HgCdTe photodiodes August 2008
A synthetic Roman Space Telescope High-Latitude Imaging Survey: simulation suite and the impact of wavefront errors on weak gravitational lensing November 2020
The High Latitude Spectroscopic Survey on the Nancy Grace Roman Space Telescope March 2022
Weak gravitational lensing shear estimation with metacalibration for the Roman High-Latitude Imaging Survey September 2022