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JWST COMPASS: Insights into the Systematic Noise Properties of NIRSpec/G395H from a Uniform Reanalysis of Seven Transmission Spectra

  • Authors: Tyler A. Gordon, Natalie M. Batalha, Natasha E. Batalha, Artyom Aguichine, Anna Gagnebin, James Kirk, Mercedes López-Morales, Annabella Meech, Nicholas Scarsdale, Johanna Teske, Nicole L. Wallack, Nicholas Wogan

Tyler A. Gordon et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 9. Principal component analysis

The complete figure set (26 images) is available in the online journal.

Principal components of the relative pixel fluxes (RPFs) for the first visit of GJ 357 b for NRS1 (left panel) and NRS2 (right panel). Left column of each panel: map of correlation coefficients between individual pixel fluxes and each principal component in the detector plane. Lighter colors indicate pixels that have a high positive correlation with the principal component, and dark colored pixels have a large negative correlation. Center column of each panel: principal components of the RPFs. Right column of each panel: power spectral density (PSD) of the principal component. The full figure set (26 images) is available.

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