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ARES.* V. No Evidence For Molecular Absorption in the HST WFC3 Spectrum of GJ 1132 b

Mugnai, L; Modirrousta-Galian, D; Edwards, B; Changeat, Q; Bouwman, J; Morello, G; Al-Refaie, A; ... Beaulieu, J-P; + view all (2021) ARES.* V. No Evidence For Molecular Absorption in the HST WFC3 Spectrum of GJ 1132 b. The Astronomical Journal , 161 (6) , Article 284. 10.3847/1538-3881/abf3c3. Green open access

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Abstract

We present a study on the spatially scanned spectroscopic observations of the transit of GJ 1132 b, a warm (~500 K) super-Earth (1.13 R⊕) that was obtained with the G141 grism (1.125–1.650 μm) of the Wide Field Camera 3 (WFC3) on board the Hubble Space Telescope. We used the publicly available Iraclis pipeline to extract the planetary transmission spectra from the five visits and produced a precise transmission spectrum. We analyzed the spectrum using the TauREx3 atmospheric retrieval code, with which we show that the measurements do not contain molecular signatures in the investigated wavelength range and are best fit with a flat-line model. Our results suggest that the planet does not have a clear primordial, hydrogen-dominated atmosphere. Instead, GJ 1132 b could have a cloudy hydrogen-dominated atmosphere, have a very enriched secondary atmosphere, be airless, or have a tenuous atmosphere that has not been detected. Due to the narrow wavelength coverage of WFC3, these scenarios cannot be distinguished yet, but the James Webb Space Telescope may be capable of detecting atmospheric features, although several observations may be required to provide useful constraints.

Type: Article
Title: ARES.* V. No Evidence For Molecular Absorption in the HST WFC3 Spectrum of GJ 1132 b
Open access status: An open access version is available from UCL Discovery
DOI: 10.3847/1538-3881/abf3c3
Publisher version: https://doi.org/10.3847/1538-3881/abf3c3
Language: English
Additional information: This version is the version of record. For information on re-use, please refer to the publisher's terms and conditions.
Keywords: Exoplanet atmospheres (487); Astronomy data analysis (1858); Hubble Space Telescope (761); Exoplanets (498
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery.ucl.ac.uk/id/eprint/10129040
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