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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 6.

Light curve for HIP 41378 obtained during sector 7 of the TESS mission. The blue points show the 2 minute cadence photometry, having only applied a simple detrending to the data using the Lightkurve module. The red points show the data when binned to a cadence of 30 minutes. Using the ephemerides and possible periods from K2 the corresponding transit times for each planet have been indicated with arrows. For planet “d” the only possible period that would result in a transit during the sector 7 baseline is that of n = 5. The black transit model shows transit shape for planet “d” based on the K2 analysis.

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