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TAU-REX I: A NEXT GENERATION RETRIEVAL CODE FOR EXOPLANETARY ATMOSPHERES

  • Authors: I. P. Waldmann, G. Tinetti, M. Rocchetto, E. J. Barton, S. N. Yurchenko, and J. Tennyson

2015 The Astrophysical Journal 802 107.

  • Provider: AAS Journals

Caption: Figure 5.

Top: Hubble/WFC3 transmission spectrum of HD 209458b (Deming et al. 2013; black). Overplotted are the principal components of the four best matching molecules binned to the resolution of the data: H2O (blue dots), CO2 (green squares), NH3 (magenta triangles), and NO (red squares). The H2O principal component is also shown at a resolution of R = 1000 (light blue). Bottom: the normalized euclidean distance between each individual component and the data. It is clear that H2O presents the best match to the data with other molecules being significantly worse.

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