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TESS full orbital phase curve of the WASP-18b system
Avi Shporer, Ian Wong, Chelsea X. Huang +18
We present a visible-light full orbital phase curve of the transiting planet WASP-18b measured by the TESS Mission. The phase curve includes the transit, secondary eclipse, and sin…
Simulating the M-R Relation from APF follow up of TESS targets: Survey design and strategies for overcoming mass biases
Jennifer Burt, Bradford P. Holden, Angie Wolfgang +1
We present simulations of multi-year RV follow up campaigns of the {\it TESS} small exoplanet yield on the Automated Planet Finder telescope, using four different schemes to sample…
Biases in Planet Occurrence Caused by Unresolved Binaries in Transit Surveys
L. G. Bouma, Kento Masuda, J. N. Winn
Wide-field surveys for transiting planets, such as the NASA Kepler and TESS missions, are usually conducted without knowing which stars have binary companions. Unresolved and unrec…
Empirical Tidal Dissipation in Exoplanet Hosts From Tidal Spin-Up
Kaloyan Penev, L. G. Bouma, Joshua N. Winn +1
Stars with hot Jupiters tend to be rotating faster than other stars of the same age and mass. This trend has been attributed to tidal interactions between the star and planet. A co…
The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package
The Astropy Collaboration, A. M. Price-Whelan, B. M. Sipőcz +134
The Astropy project supports and fosters the development of open-source and openly-developed Python packages that provide commonly-needed functionality to the astronomical communit…