Mass determination of two Jupiter-sized planets orbiting slightly evolved stars: TOI-2420 b and TOI-2485 b

Ilaria Carleo, Oscar Barrágan, Carina M. Persson, Malcolm Fridlund, Kristine W.F. Lam, Sergio Messina, Davide Gandolfi, Alexis M.S. Smith, Marshall C. Johnson, William Cochran, Hannah L.M. Osborne, Rafael Brahm, David R. Ciardi, Karen A. Collins, Mark E. Everett, Steven Giacalone, Eike W. Guenther, Artie Hatzes, Coel Hellier, Jonathan HornerPetr Kabáth, Judith Korth, Phillip Macqueen, Thomas Masseron, Felipe Murgas, Grzegorz Nowak, Joseph E. Rodriguez, Cristilyn N. Watkins, Rob Wittenmyer, George Zhou, Carl Ziegler, Allyson Bieryla, Patricia T. Boyd, Catherine A. Clark, Courtney D. Dressing, Jason D. Eastman, Jan Eberhardt, Michael Endl, Nestor Espinoza, Michael Fausnaugh, Natalia M. Guerrero, Thomas Henning, Katharine Hesse, Melissa J. Hobson, Steve B. Howell, Andrés Jordán, David W. Latham, Michael B. Lund, Ismael Mireles, Norio Narita, Marcelo Tala Pinto, Teznie Pugh, Samuel N. Quinn, George Ricker, David R. Rodriguez, Felipe I. Rojas, Mark E. Rose, Alexander Rudat, Paula Sarkis, Arjun B. Savel, Martin Schlecker, Richard P. Schwarz, Sara Seager, Avi Shporer, Jeffrey C. Smith, Keivan G. Stassun, Chris Stockdale, Trifon Trifonov, Roland Vanderspek, Joshua N. Winn, Duncan Wright

Research output: Contribution to journalArticlepeer-review

Original languageEnglish
Article numberA18
JournalAstronomy and Astrophysics
Volume690
DOIs
StatePublished - Oct 1 2024

ASJC Scopus Subject Areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Planets and satellites: detection
  • Planets and satellites: gaseous planets

Cite this