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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 7.

Top: star location offsets in pixel coordinates for an 8 × 8 grid, arranged by individual SCA. The black line is all stars, and the purple line is stars with 19 < mtruth < 21.5. Bottom: the same for the J129 band. This plot is formatted to reflect Roman’s detector shape and SCA arrangement. σ is the standard deviation of the purple line. We choose to show the R062 and J129 bands to illustrate this discussion point (Figures 4 and 10) because they have the largest and smallest differences, respectively, in their x- and y-coordinate recovery precision (Table 2).

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