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Increasing Sensitivity to Trailed Solar System Objects in Archival JWST NIRCam Imaging with Group Differencing

  • Authors: Anthony Girmenia, Stanimir Metchev

Anthony Girmenia and Stanimir Metchev 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 7.

Flux agreement between ramp-fit and group-difference estimates for our candidate moving sources (see Tables 3 and 4). Only sources with SNR > 5 in both the ramp-fit and group-differenced images are plotted here. All magnitudes agree within their uncertainties, demonstrating that flux is conserved across both image calibrations.

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