Published October 8, 2020
| Version Version 1.0
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Atmosphere of HAT-P-41b Revealed - Supplemental Figures
Contributors
Project member (4):
- 1. School of Physics, University of Bristol, H.H. Wills Physics Laboratory, Tyndall Avenue, Bristol BS8 1TL, UK
- 2. Department of Astronomy and Carl Sagan Institute, Cornell University, 122 Sciences Drive, Ithaca, NY 14853, USA
- 3. School of Physical Sciences, Open University, Walton Hall, Kents Hill, Milton Keynes MK7 6AA, UK
Description
Supplemental Figures for 'Into the UV: The Atmosphere of the Hot Jupiter HAT-P-41b Revealed" (Lewis et al. 2020, ApJL 902:L19).
Contains retrieval posteriors, spectra, abundances, comparisons between retrieved pressure-temperature profiles, and the lightcurve analysis for Hubble's WFC3 G141 data of HAT-P-41b. These figures support the analysis of HAT-P-41b's atmosphere presented in the main manuscript.
Files
ATMO_HAT-P-41b_eqchem_posterior_jitter.png
Files
(46.7 MB)
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Additional details
Related works
- Is supplement to
- Journal article: 10.3847/2041-8213/abb77f (DOI)