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The HD 60779 Planetary System: A Transiting Sub-Neptune on a 30 Day Orbit and a More Massive Outer World

Authors: Victoria DiTomasso, David Charbonneau, Andrew Vanderburg, Mercedes López- Morales, Shreyas Vissapragada, Annelies Mortier, Thomas G. Wilson, Elyse Incha, Andrew Collier Cameron, Luca Malavolta, Lars A. Buchhave, David W. Latham, Matteo Pinamonti, Stephanie Striegel, Michael Fausnaugh, Luke Bouma, Ben Falk, Robert Aloisi, Xavier Dumusque, A. Anna John, Ben S. Lakeland, A. F. Martínez Fiorenzano, Luca Naponiello, Belinda Nicholson, Emily K. Pass, Francesco Alfonso Pepe, Federica Rescigno, Alessandro Sozzetti, Daisy A. Turner, Saul A. Rappaport, Mark Omohundro, Brian P. Powell, Robert Gagliano, Thomas L. Jacobs, Veselin B. Kostov, Martti H. Kristiansen, Daryll M. LaCourse, Allan R. Schmitt, Hans Martin Schwengeler, Ivan A. Terentev

Victoria DiTomasso et al 2026 The Astronomical Journal 172 .

Provider: AAS Journals

Caption: Figure 1.

HARPS-N DRS 3.3.12 data products. The left column shows the time series of the RVs, followed by the various activity indicators. The middle column shows those values plotted with respect to the RV. The Pearson r correlation coefficient is noted in the lower right of each subpanel. The right column shows the periodograms of these measurements. All of the significant periodicities (FAP < 0.0001) are marked with vertical lines in all of the panels. We have excluded four contrast outliers, four SMW outliers, and four Ca II H and K outliers using 3σ clipping.

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