Image Details
Caption: Figure 2.
Left: a median combination of our observations of TOI 700 d (upper panel) and e (lower panel). The dashed/dotted lines show our extraction apertures. Right: an observation taken with the F277W filter. As only the reddest end of order 1 is transmitted, this filter reveals background contaminants. We carefully selected our aperture position angle constraints so that only a few contaminants are present within our apertures; we mask these wavelengths before producing our white-light curves.
© 2026. The Author(s). Published by the American Astronomical Society.