Figure 8 from HATS-36b and 24 Other Transiting/Eclipsing Systems from the HATSouth-K2 Campaign 7 Program

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HATS-36b and 24 Other Transiting/Eclipsing Systems from the HATSouth-K2 Campaign 7 Program

Authors: D. Baylisss, J. D. Hartman, G. Zhou, G. Á. Bakos, A. Vanderburg, J. Bento, L. Mancini, S. Ciceri, R. Brahm, A. Jordán, N. Espinoza, M. Rabus, T. G. Tan, K. Penev, W. Bhatti, M. de Val-Borro, V. Suc, Z. Csubry, Th. Henning, P. Sarkis, J. Lázár, I. Papp, and P. Sári

2018 The Astronomical Journal 155 119.

Provider: AAS Journals

Caption: Figure 8.

The power spectrum from a Lomb–Scargle analysis of the HATSouth photometry (blue solid line) and the K2 photometry (red dashed line) for HATS-36. The peak at ∼14 days is the likely rotational period of the star and is prominent in both data sets.

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