Linking atmospheric chemistry of the hot Jupiter HD 209458b to its formation location through infrared transmission and emission spectra

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作者：
Dash, Spandan [1 ,2 ,3 ]
Majumdar, Liton [2 ,3 ]
Willacy, Karen [4 ]
Tsai, Shang-Min [5 ]
Turner, Neal [4 ]
Rimmer, P.B. [6 ,7 ,8 ]
Gudipati, Murthy S. [4 ]
Lyra, Wladimir [9 ]
Bhardwaj, Anil [10 ]
机构：
[1] Department of Physics, University of Warwick, West Midlands, Coventry,CV4 7AL, United Kingdom
[2] School of Earth and Planetary Sciences, National Institute of Science Education and Research, Odisha, Jatni,752050, India
[3] Homi Bhabha National Institute, Training School Complex, Anushaktinagar, Mumbai,400094, India
[4] Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena,CA,91109, United States
[5] Atmospheric, Ocean, and Planetary Physics, Department of Physics, University of Oxford, Oxford,OX1 3PU, United Kingdom
[6] MRC Laboratory of Molecular Biology, Francis Crick Ave, Cambridge,CB2 0QH, United Kingdom
[7] Astrophysics Group Cavendish Laboratory, JJ Thomson Ave, Cambridge,CB3 0HE, United Kingdom
[8] Department of Earth Sciences, University of Cambridge, Downing St, Cambridge,CB2 3EQ, United Kingdom
[9] Department of Astronomy, New Mexico State University, PO BOX 30001, MSC 4500, Las Cruces,NM,88003-8001, United States
[10] Physical Research Laboratory, Ahmedabad,380009, India
来源：
arXiv | 2022年
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摘要：
Atmospheric chemistry
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