Figure 1 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 1.

Band-integrated light curve and residuals. (a) Raw light curve (black points) and model (red). (b) Raw orbit-to-orbit residuals showing the gradient difference between HST orbit 1 and orbits 2–4. (c) Light curve corrected by the systematic model and the best-fit transit model (red). (d) Residuals in parts per million (ppm) of corrected light curve compared to the transit model (red dashed line).

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