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Morphological and Star Formation Properties of Cosmic Noon Massive Quiescent Galaxies

  • Authors: Vaidik Prasal, Yogesh Wadadekar, Pralay Biswas, Rashi Jain

Vaidik Prasal et al 2026 The Astrophysical Journal 1009 .

  • Provider: AAS Journals

Caption: Figure 5.

Two-component pysersic fits for the galaxies in our sample in the F444W filter (4″ cutouts). The panels display the original images, the best-fit models, and the resulting residual maps. The color scale limits (vmin and vmax) for the residual plots are set to ±0.1 (in 10 nJy), where blue regions indicate less flux than the model and red regions indicate excess flux. The average absolute residual is 1.48% ± 0.67%, with values ranging from 0.16% to 10.25%. The standard deviation of the mean is calculated via bootstrapping for 1000 iterations.

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