Figure 3 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 3.

Left: unbinned ground-based follow-up transit light curves of HATS579-037. Plots as for Figure 2. The over-plotted model is based on a global fit of all available data, and accounts for differences in limb darkening between the R- and i-bands, but assumes all other light curve parameters are the same. The poor fit of this model shows clear differences in the observed transit depths between the R-band and i-band observations, which allow us to classify this candidate as a eclipsing binary.

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