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Asteroseismology of the Multiplanet System K2-93

  • Authors: Mikkel N. Lund, Emil Knudstrup, Víctor Silva Aguirre, Sarbani Basu, Ashley Chontos, Carolina Von Essen, William J. Chaplin, Allyson Bieryla, Luca Casagrande, Andrew Vanderburg, Daniel Huber, Stephen R. Kane, Simon Albrecht, David W. Latham, Guy R. Davies, Juliette C. Becker, and Joseph E. Rodriguez

2019 The Astronomical Journal 158 248.

  • Provider: AAS Journals

Caption: Figure 2.

Power density spectrum (PDS; left) and échelle diagram (right) of HIP 41378. The black line shows a smoothed version of the PDS and the red dashed line indicates the value of ﹩{\nu }_{\max }﹩. The insert in the PDS shows the ﹩\mathrm{PS}\otimes \ \mathrm{PS}﹩ of a region centered on the measured ﹩{\nu }_{\max }﹩; the peak in the ﹩\mathrm{PS}\otimes \ \mathrm{PS}﹩ marked by a dashed red line gives the identified value for ﹩{\rm{\Delta }}\nu /2﹩, while the dotted line shows the value of ﹩{\rm{\Delta }}\nu /4﹩.

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