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Initial Characterization of Stellar Photometry of Roman Images from the OpenUniverse Simulations

  • Authors: L. Aldoroty, D. Scolnic, A. Kannawadi, R. A. Knop, B. M. Rose, R. Hounsell, M. A. Troxel

L. Aldoroty et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 11.

GalSim PSFs, unconvolved with the Roman pixel response, at the center of each SCA. All PSFs are oversampled by a factor of 9. This plot is formatted to reflect Roman’s detector shape and SCA arrangement. Note that for the bottom two rows of the detector, the x-axis is defined such that the origin is at the bottom-right corner of the detectors, and positive x points left (M. A. Troxel et al. 2023).

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