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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 4.

Two-component pysersic fits for the galaxies in our sample in the F200W filter (4″ cutouts). The panels display the original images, the median 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 4.16% ± 1.39%, with values ranging from 0.38% to 22.09%. The standard deviation of the mean is calculated via bootstrapping for 1000 iterations.

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