The HUSTLE Program: The UV to Near-infrared HST WFC3/UVIS G280 Transmission Spectrum of WASP-127b

Ultraviolet wavelengths offer unique insights into aerosols in exoplanetary atmospheres. However, only a handful of exoplanets have been observed in the ultraviolet to date. Here, we present the ultraviolet-visible transmission spectrum of the inflated hot Jupiter WASP-127b. We observed one transit...

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Veröffentlicht in:	The Astronomical journal 2025-01, Vol.169 (1), p.23
Hauptverfasser:	Boehm, V. A., Lewis, N. K., Fairman, C. E., Moran, S. E., Gascón, C., Wakeford, H. R., Alam, M. K., Alderson, L., Barstow, J., Batalha, N. E., Grant, D., López-Morales, M., MacDonald, R. J., Marley, Mark S., Ohno, K.
Format:	Artikel
Sprache:	eng
Schlagworte:	Aerosols Atmospheric composition Broadband Exoplanet atmospheres Exoplanets Extrasolar gaseous giant planets Extrasolar planets Gas giant planets High altitude Hubble Space Telescope Jupiter Near infrared radiation Opacity Planetary atmospheres Space telescopes Transit Transmission spectroscopy Ultraviolet astronomy Ultraviolet spectra Wavelengths
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