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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 4.

Left: the modified median absolute deviation (﹩\hat{\sigma }﹩), assuming a normal distribution, of the fractional difference between truth catalog flux and the fit PSF photometry flux as a function of grid element size in pixels. Center: ﹩\hat{\sigma }﹩, assuming a normal distribution, of the difference between truth catalog pixel coordinates and fit pixel coordinates. Right: ﹩\hat{\sigma }﹩ of the fractional flux differences from the left panel compared to the pixel locations in the center panel. Circular markers with solid lines correspond to the x-coordinates, and triangles with dashed lines correspond to y-coordinates. The shaded purple region represents <1% flux precision. This figure corresponds with the results in Table 2.

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