TOI-3493 b: A planet with a Neptune-like density transiting a bright G0-type star

P. Chaturvedi, E. Goffo, D. Gandolfi, C. M. Persson, A. P. Hatzes, G. Nowak, A. Bonfanti, A. Bieryla, W. D. Cochran, K. A. Collins, S. B. Fajardo-Acosta, S. B. Howell, J. M. Jenkins, J. Korth, J. Livingston, E. Pallé, S. N. Quinn, R. P. Schwarz, S. Seager, A. ShporerK. G. Stassun, S. Striegel, V. Van Eylen, C. N. Watkins, J. N. Winn, C. Ziegler

Research output: Contribution to journalArticlepeer-review

Original languageEnglish
Article numberA169
JournalAstronomy and Astrophysics
Volume697
DOIs
StatePublished - May 1 2025

ASJC Scopus Subject Areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Planets and satellites: detection
  • Stars: individual: TOI-3493
  • Stars: solar-type
  • Techniques: photometric
  • Techniques: radial velocities

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