2 code implementations • CIKM 2023 • Bin Wu, Xinyu Yao, Boyan Zhang, Kuo-Ming Chao, Yinsheng Li
However, researches on addressing the heterophily problem in the spectral domain are still limited due to a lack of understanding of spectral energy distribution in graphs with heterophily.
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no code implementations • 20 Sep 2017 • Robert J. Siverd, Karen A. Collins, George Zhou, Samuel N. Quinn, B. Scott Gaudi, Keivan G. Stassun, Marshall C. Johnson, Allyson Bieryla, David W. Latham, David R. Ciardi, Joseph E. Rodriguez, Kaloyan Penev, Marc Pinsonneault, Joshua Pepper, Jason D. Eastman, Howard Relles, John F. Kielkopf, Joao Gregorio, Thomas E. Oberst, Giulio Francesco Aldi, Gilbert A. Esquerdo, Michael L. Calkins, Perry Berlind, Courtney D. Dressing, Rahul Patel, Daniel J. Stevens, Thomas G. Beatty, Michael B. Lund, Jonathan Labadie-Bartz, Rudolf B. Kuhn, Knicole D. Colón, David James, Xinyu Yao, John A. Johnson, Jason T. Wright, Nate McCrady, Robert A. Wittenmyer, Samson A. Johnson, David H. Sliski, Eric L. N. Jensen, David H. Cohen, Kim K. McLeod, Matthew T. Penny, Michael D. Joner, Denise C. Stephens, Steven Villanueva Jr., Roberto Zambelli, Christopher Stockdale, Phil Evans, Thiam-Guan Tan, Ivan A. Curtis, Phillip A. Reed, Mark Trueblood, Patricia Trueblood
We confirm the planetary nature of the companion via a combination of radial velocities, which limit the mass to $< 4. 1\,\mathrm{M_J}$ $(3\sigma)$, and a clear Doppler tomography signal, which indicates a retrograde projected spin-orbit misalignment of $\lambda = -179. 7^{+3. 7}_{-3. 8}$ degrees.
Earth and Planetary Astrophysics