no code implementations • 11 Feb 2021 • Elisabeth R. Newton, Andrew W. Mann, Adam L. Kraus, John H. Livingston, Andrew Vanderburg, Jason L. Curtis, Pa Chia Thao, Keith Hawkins, Mackenna L. Wood, Aaron C. Rizzuto, Abderahmane Soubkiou, Benjamin M. Tofflemire, George Zhou, Ian J. M. Crossfield, Logan A. Pearce, Karen A. Collins, Dennis M. Conti, Thiam-Guan Tan, Steven Villeneuva, Alton Spencer, Diana Dragomir, Samuel N. Quinn, Eric L. N. Jensen, Kevin I. Collins, Chris Stockdale, Ryan Cloutier, Coel Hellier, Zouhair Benkhaldoun, Carl Ziegler, César Briceño, Nicholas Law, Björn Benneke, Jessie L. Christiansen, Varoujan Gorjian, Stephen R. Kane, Laura Kreidberg, Farisa Y. Morales, Michael W Werner, Joseph D. Twicken, Alan M. Levine, David R. Ciardi, Natalia M. Guerrero, Katharine Hesse, Elisa V. Quintana, Bernie Shiao, Jeffrey C. Smith, Guillermo Torres, George R. Ricker, Roland Vanderspek, Sara Seager, Joshua N. Winn, Jon M. Jenkins, David W. Latham
Young exoplanets can offer insight into the evolution of planetary atmospheres, compositions, and architectures.
Earth and Planetary Astrophysics Solar and Stellar Astrophysics
1 code implementation • 16 Nov 2018 • Andrew W. Mann, Trent Dupuy, Adam L. Kraus, Eric Gaidos, Megan Ansdell, Michael Ireland, Aaron C. Rizzuto, Chao-Ling Hung, Jason Dittmann, Samuel Factor, Gregory Feiden, Raquel A. Martinez, Dary Ruiz-Rodriguez, Pa Chia Thao
The result can be used to determine masses of single stars with a precision of 2-3%, which we confirm by a comparison to dynamical masses from the literature.
Solar and Stellar Astrophysics