Figure 5 from HATS-37Ab and HATS-38b: Two Transiting Hot Neptunes in the Desert

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HATS-37Ab and HATS-38b: Two Transiting Hot Neptunes in the Desert

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

2020 The Astronomical Journal 160 222.

Provider: AAS Journals

Caption: Figure 5.

Top: RV observations of HATS-37 plotted against time. The solid line shows the best-fit model including a linear trend and the Keplerian orbital variation of the host star due to the planet HATS-37Ab. As in Figure 1, the RV model plotted here is not corrected for dilution from the unresolved stellar component HATS-37B. The corrected semiamplitude of the orbit is ∼20% larger than what is shown. Bottom: RV residuals from the best-fit model plotted against time.

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