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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 7.

Period–radius diagram for the population of well-characterized transiting planets. The points corresponding to HATS-37Ab and HATS-38b are indicated with dotted black lines. The dashed cyan lines mark the boundaries of the Neptune desert as defined by Mazeh et al. (2016). The points are color-coded according to the metallicity of the host star.

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