Image Details
Caption: Figure 3.
The plots of rms vs. bin size for both detectors for both reductions. We show the actual noise for NRS1 in blue and for NRS2 in red; in the absence of red noise, the residuals would follow the correspondingly colored solid lines. We see residual correlated noise in both detectors for both reductions of both visits.
© 2026. The Author(s). Published by the American Astronomical Society.