The Unrealised Interdisciplinary Advantage of Observing High Mass Transiting Exoplanets and Brown Dwarfs — Strategic Exoplanet Initiatives with HST and JWST White Paper
We advocate for further prioritisation of atmospheric characterisation observations of high mass transiting exoplanets and brown dwarfs.
This population acts as a unique comparative sample to the directly imaged exoplanet and brown dwarf populations, of which a range of JWST characterisation observations are planned.
In contrast, only two observations of transiting exoplanets in this mass regime were performed in Cycle 1, and none are planned for Cycle 2. Such observations will: improve our understanding of how irradiation influences high gravity atmospheres, provide insights towards planetary formation and evolution across this mass regime, and exploit JWST’s unique potential to characterise exoplanets across the known population.
Aarynn L. Carter, Munazza. K. Alam, Thomas Beatty, Sarah Casewell, Katy L. Chubb, Kielan Hoch, Nikole Lewis, Joshua D. Lothringer, Elena Manjavacas, Sarah E. Moran, Hannah R. Wakeford
Comments: 4 pages, 2 figures. This white paper was submitted following a call from the “Working Group on Strategic Exoplanet Initiatives with HST and JWST” (this https URL, final report in https://doi.org/10.48550/arXiv.2404.02932)
Subjects: Instrumentation and Methods for Astrophysics (astro-ph.IM); Earth and Planetary Astrophysics (astro-ph.EP); Solar and Stellar Astrophysics (astro-ph.SR)
Cite as: arXiv:2408.07723 [astro-ph.IM] (or arXiv:2408.07723v1 [astro-ph.IM] for this version)
https://doi.org/10.48550/arXiv.2408.07723
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Submission history
From: Aarynn Carter Dr
[v1] Wed, 14 Aug 2024 13:33:07 UTC (1,088 KB)
https://arxiv.org/abs/2408.07723
Astrobiology,