The HUSTLE Program: The UV to Near-IR Transmission Spectrum of the Hot Jupiter KELT-7b

The HUSTLE Program: The UV to Near-IR Transmission Spectrum of the Hot Jupiter KELT-7b

The ultraviolet and optical wavelength ranges have proven to be a key addition to infrared observations of exoplanet atmospheres because they offer unique insights into the properties of clouds and hazes and are sensitive to signatures of disequilibrium chemistry. Here, we present the 0.2–0.8 μ m tr...

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Bibliographic Details
Main Authors: C. Gascón, M. López-Morales, R. J. MacDonald, J. K. Barstow, V. A. Boehm, H. R. Wakeford, M. K. Alam, L. Alderson, N. E. Batalha, C. E. Fairman, D. Grant, N. K. Lewis, M. S. Marley, S. E. Moran, K. Ohno, G. Anglada-Escudé, I. Ribas
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astronomical Journal
Subjects:
Exoplanets
Hot Jupiters
Exoplanet atmospheres
Online Access:https://doi.org/10.3847/1538-3881/ade67e
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https://doi.org/10.3847/1538-3881/ade67e

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