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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 7.

GLS periodograms for HIP 8152 are shown in black. The vertical blue and orange lines mark the orbital periods of planets b and c, respectively. The dashed horizontal line indicates the 0.1% FAP threshold (Baluev 2008). We compute the GLS periodogram of the RV window function with a minimum period slightly longer than 1 day to avoid the strong nightly alias, which otherwise skews the y-axis scale.

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