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TOI-1408: Discovery and Photodynamical Modeling of a Small Inner Companion to a Hot Jupiter Revealed by Transit Timing Variations

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By Hanna M, Van Eylen
| Caltech
Acknowledgement We thank the anonymous referee for the timely and positive feedback. This work was supported by the KESPRINT collaboration, an international consortium devoted to the characterization and research of exoplanets discovered with space-based missions (https://kesprint.science/). This Letter includes data collected with the TESS mission, obtained from the MAST data archive at the Space Telescope Science Institute (STScI). The specific data can be obtained here: doi: 10.17909/en2q-wj40.
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