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The TESS-Keck Survey. XVI. Mass Measurements for 12 Planets in Eight Systems

  • Authors: Joseph M. Akana Murphy, Natalie M. Batalha, Nicholas Scarsdale, Howard Isaacson, David R. Ciardi, Erica J. Gonzales, Steven Giacalone, Joseph D. Twicken, Anne Dattilo, Tara Fetherolf, Ryan A. Rubenzahl, Ian J. M. Crossfield, Courtney D. Dressing, Benjamin Fulton, Andrew W. Howard, Daniel Huber, Stephen R. Kane, Erik A. Petigura, Paul Robertson, Arpita Roy, Lauren M. Weiss, Corey Beard, Ashley Chontos, Fei Dai, Malena Rice, Judah Van Zandt, Jack Lubin, Sarah Blunt, Alex S. Polanski, Aida Behmard, Paul A. Dalba, Michelle L. Hill, Lee J. Rosenthal, Casey L. Brinkman, Andrew W. Mayo, Emma V. Turtelboom, Isabel Angelo, Teo Močnik, Mason G. MacDougall, Daria Pidhorodetska, Dakotah Tyler, Molly R. Kosiarek, Rae Holcomb, Emma M. Louden, Lea A. Hirsch, Emily A. Gilbert, Jay Anderson, Jeff A. Valenti

Joseph M. Akana Murphy et al 2023 The Astronomical Journal 166 .

  • Provider: AAS Journals

Caption: Figure 9.

The S HK portion of the joint model for HD 6061, in which GPs with some shared hyperparameters are simultaneously fit to the RVs and the Keck-HIRES S HK values. The GP kernel is described in Section 9.3. The best-fitting value of the GP period is P rot = 13.9 ± 1.5 days. See Figure 23 for the photometry and RV portions of this joint model. The GP posterior prediction is shown as the blue line surrounded by a 1σ error envelope. The Keck-HIRES S HK values are shown as the black points with 1σ errors, where the measurement error on each S HK value has been added in quadrature with the a jitter term that has been fit to the data. Residuals are shown in the bottom panel.

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