Figure 3 from HST PanCET Program: A Cloudy Atmosphere for the Promising JWST Target WASP-101b

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HST PanCET Program: A Cloudy Atmosphere for the Promising JWST Target WASP-101b

Authors: H. R. Wakeford, K. B. Stevenson, N. K. Lewis, D. K. Sing, M. López-Morales, M. Marley, T. Kataria, A. Mandell, G. E. Ballester, J. Barstow, L. Ben-Jaffel, V. Bourrier, L. A. Buchhave, D. Ehrenreich, T. Evans, A. García Muñoz, G. Henry, H. Knutson, P. Lavvas, A. Lecavelier des Etangs, N. Nikolov, and J. Sanz-Forcada

2017 The Astrophysical Journal Letters 835 L12.

Provider: AAS Journals

Caption: Figure 3.

Transmission spectrum of WASP-101b from our common-mode analysis (black points) and using marginalization (gray squares). We use the common-mode transmission spectrum and fit for the best 1D isothermal model (Fortney et al. 2010), which has T = 1250 K and a flat cloud deck ×100 the hydrogen cross-section (red). The model in blue shows the expected absorption feature for a clear atmosphere at the same temperature. The dashed line shows the null hypothesis.

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