Figure 6 from HATS-37Ab and HATS-38b: Two Transiting Hot Neptunes in the Desert

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 6.

Mass–radius diagram for the population of well-characterized transiting planets (Southworth 2011). The points corresponding to HATS-37Ab and HATS-38b are indicated with dashed lines. The color represents the equilibrium temperature of the planet, while the size scales down with the transmission spectroscopy metric as defined by Kempton et al. (2018). The dashed gray lines correspond to isodensity curves for 0.3, 3 and 30 g cm⁻³, respectively.

Other Images in This Article

Copyright and Terms & Conditions