Image Details
Caption: Figure 10.
Eclipse depths for NGTS-EB-8 derived for the primary (orange circles) and secondary (green squares) eclipses in parts per thousand. The uncertainties are the 99.7% (∼3σ) percentiles of the derived posteriors. Left panel: eclipse depths for instruments where we detect both the primary and secondary eclipses. The weighted mean for both eclipses is shown as a dashed line, with shaded regions indicating the weighted uncertainty. Right panel: primary eclipse depths for the SAAO and ATLAS-c observations.
© 2025. The Author(s). Published by the American Astronomical Society.