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A New Third Planet and the Dynamical Architecture of the HD 33142 Planetary System

  • Authors: Trifon Trifonov, Anna Wollbold, Martin Kürster, Jan Eberhardt, Stephan Stock, Thomas Henning, Sabine Reffert, R. Paul Butler, Steven S. Vogt, Ansgar Reiners, Man Hoi Lee, Bertram Bitsch, Mathias Zechmeister, Florian Rodler, Volker Perdelwitz, Lev Tal-Or, Jan Rybizki, Paul Heeren, Davide Gandolfi, Oscar Barragán, Olga Zakhozhay, Paula Sarkis, Marcelo Tala Pinto, Diana Kossakowski, Vera Wolthoff, Stefan S. Brems, Vera Maria Passegger

Trifon Trifonov et al 2022 The Astronomical Journal 164 .

  • Provider: AAS Journals

Caption: Figure 2.

MLP of the combined RV data from HARPS, HIRES, and FEROS, as well as stellar activity indicators. The horizontal lines correspond to the FAP levels of 10% (dotted line), 1% (dotted–dashed line), and 0.1% (dashed line). The orbital periods of the planets are indicated as vertical dashed blue lines and the estimate for the rotation period by Jofré et al. (2015) is shown as a red dashed line, while the red shaded area denotes its uncertainties (see Table 1).

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