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Transmission spectroscopy with VLT FORS2: a featureless spectrum for the low-density transiting exoplanet WASP-88b

Spyratos, Petros; Nikolov, Nikolay; Southworth, John; Constantinou, Savvas; Madhusudhan, Nikku; Carter, Aarynn L; de Mooij, Ernst J W; Fortney, Jonathan J; Gibson, Neale P; Goyal, Jayesh M; Helling, Christiane; Mayne, Nathan J; Mikal-Evans, Thomas

Transmission spectroscopy with VLT FORS2: a featureless spectrum for the low-density transiting exoplanet WASP-88b Thumbnail


Authors

Petros Spyratos

Nikolay Nikolov

Savvas Constantinou

Nikku Madhusudhan

Aarynn L Carter

Ernst J W de Mooij

Jonathan J Fortney

Neale P Gibson

Jayesh M Goyal

Christiane Helling

Nathan J Mayne

Thomas Mikal-Evans



Abstract

We present ground-based optical transmission spectroscopy of the low-density hot Jupiter WASP-88b covering the wavelength range 4413 - 8333 Å with the FORS2 spectrograph on the Very Large Telescope. The FORS2 white light curves exhibit a significant time-correlated noise which we model using a Gaussian Process and remove as a wavelength-independent component from the spectroscopic light curves. We analyse complementary photometric observations from the Transiting Exoplanet Survey Satellite and refine the system properties and ephemeris. We find a featureless transmission spectrum with increased absorption towards shorter wavelengths. We perform an atmospheric retrieval analysis with the aura code, finding tentative evidence for haze in the upper atmospheric layers and a lower likelihood for a dense cloud deck. Whilst our retrieval analysis results point toward clouds and hazes, further evidence is needed to definitively reject a clear-sky scenario.

Journal Article Type Article
Acceptance Date Jun 24, 2021
Online Publication Date Jul 5, 2021
Publication Date 2021-09
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 506
Issue 2
Pages 2853-2870
DOI https://doi.org/10.1093/mnras/stab1847
Keywords methods: data analysis, techniques: spectroscopic, planets and satellites: atmospheres, stars: individual: WASP-88, planetary systems
Publisher URL https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stab1847/6315343

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