no code implementations • 19 Feb 2024 • Greg Olmschenk, Richard K. Barry, Stela Ishitani Silva, Brian P. Powell, Ethan Kruse, Jeremy D. Schnittman, Agnieszka M. Cieplak, Thomas Barclay, Siddhant Solanki, Bianca Ortega, John Baker, Yesenia Helem Salinas Mamani
The Transiting Exoplanet Survey Satellite (TESS) mission measured light from stars in ~85% of the sky throughout its two-year primary mission, resulting in millions of TESS 30-minute cadence light curves to analyze in the search for transiting exoplanets.
no code implementations • 26 Jan 2021 • Greg Olmschenk, Stela Ishitani Silva, Gioia Rau, Richard K. Barry, Ethan Kruse, Luca Cacciapuoti, Veselin Kostov, Brian P. Powell, Edward Wyrwas, Jeremy D. Schnittman, Thomas Barclay
We present a convolutional neural network, which we train to identify planetary transit signals and dismiss false positives.
1 code implementation • 24 Jul 2019 • Aaron Hamann, Benjamin T. Montet, Daniel C. Fabrycky, Eric Agol, Ethan Kruse
In Campaign 5 data, a single planet was discovered with an orbital period of $2. 6$~days and large transit timing variations due to an unknown perturber.
Earth and Planetary Astrophysics
1 code implementation • 17 Feb 2017 • Rodrigo Luger, Ethan Kruse, Daniel Foreman-Mackey, Eric Agol, Nicholas Saunders
On average, EVEREST 2. 0 light curves have 10-20% higher photometric precision than those in the previous version, yielding the highest precision light curves at all Kp magnitudes of any publicly available K2 catalog.
Instrumentation and Methods for Astrophysics Earth and Planetary Astrophysics
1 code implementation • 2 Jul 2016 • Rodrigo Luger, Eric Agol, Ethan Kruse, Rory Barnes, Andrew Becker, Daniel Foreman-Mackey, Drake Deming
We present EVEREST, an open-source pipeline for removing instrumental noise from K2 light curves.
Earth and Planetary Astrophysics
