Image Details
Caption: Figure A1.
Left: comparison of uncertainties in the 100th spectroscopic lightcurve from Eureka! and exoTEDRF. Right: same comparison for the white lightcurves. exoTEDRF shows mostly constant uncertainties with occasional large fluctuations. In the white lightcurves, the fluctuations dominate, reducing the difference between the two pipelines.
© 2026. The Author(s). Published by the American Astronomical Society.