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

Abstract 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 of WASP-127b with WFC3/UVIS G280 as part of the Hubble Ultraviolet-optical Survey of Transiting Legacy Exoplanets, obtaining a transmission spectrum from 200 to 800 nm. Our reductions yielded a broadband transit depth precision of 91 ppm and a median precision of 240 ppm across 59 spectral channels. Our observations are suggestive of a high-altitude cloud layer with forward modeling showing they are composed of submicron particles and retrievals indicating a high-opacity patchy cloud. While our UVIS/G280 data only offer weak evidence for Na, adding archival Hubble Space Telescope (HST) WFC3/IR and STIS observations raises the overall Na detection significance to 4.1 σ . Our work demonstrates the capabilities of HST WFC3/UVIS G280 observations to probe the aerosols and atmospheric composition of transiting hot Jupiters with comparable precision to HST STIS.

Authors

Publication Details

Journal
The Astronomical Journal
Published
2024-12-12
DOI
https://doi.org/10.3847/1538-3881/ad8dde
Citations
9
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
2.98

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article

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

Natasha E. Batalha, David Grant, Carlos Gascón, Mercedes López‐Morales et al.
9 citations
The Astronomical Journal
Stellar, planetary, and galactic studies
2.98
article

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

Natasha E. Batalha, David Grant, Carlos Gascón, Mercedes López‐Morales, Munazza K. Alam, Kazumasa Ohno, Nikole K. Lewis, Ryan J. MacDonald, Sarah E. Moran, J. K. Barstow, Lili Alderson, Mark S. Marley, Hannah R. Wakeford, Charlotte Fairman, V. A. Boehm
article en
9 citations

Abstract

Abstract 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 of WASP-127b with WFC3/UVIS G280 as part of the Hubble Ultraviolet-optical Survey of Transiting Legacy Exoplanets, obtaining a transmission spectrum from 200 to 800 nm. Our reductions yielded a broadband transit depth precision of 91 ppm and a median precision of 240 ppm across 59 spectral channels. Our observations are suggestive of a high-altitude cloud layer with forward modeling showing they are composed of submicron particles and retrievals indicating a high-opacity patchy cloud. While our UVIS/G280 data only offer weak evidence for Na, adding archival Hubble Space Telescope (HST) WFC3/IR and STIS observations raises the overall Na detection significance to 4.1 σ . Our work demonstrates the capabilities of HST WFC3/UVIS G280 observations to probe the aerosols and atmospheric composition of transiting hot Jupiters with comparable precision to HST STIS.

The Astronomical JournalVol. 169(1)
National Aeronautics and Space Administration, California Institute of Technology, Space Telescope Science Institute, Government of the United Kingdom, UK Research and Innovation, University of Bristol, Generalitat de Catalunya, HORIZON EUROPE Framework Programme, Science and Technology Facilities Council, Agència de Gestió d'Ajuts Universitaris i de Recerca
Openalex Percentile: Top 9%
Stellar, planetary, and galactic studies
2.98
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