Robin Baeyens

Abstract: Funding: LC acknowledges funding by DLR grant 50OR1804. RB is PhD fellow of the Research Foundation – Flanders (FWO). LD acknowledges support from the ERC consolidator grant 646758 AEROSOL and the FWO Research Project grant G086217N. OV thanks the CNRS/INSU Programme National de Planetologie (PNP) and CNES for funding support. PM acknowledges support from the European Research Council under the European Union’s Horizon 2020 research and innovation programme under grant agreement 6945713. PS acknowledges the support from the Swiss National Science Foundation under grant BSSGI0155816 ‘PlanetsInTime’. Parts of this work have been carried out within the framework of the NCCR PlanetS supported by the Swiss National Science Foundation.

TL;DR: In this article, the atmospheric characterization of three large, gaseous planets: WASP-127 b, WASP79 b, and WASP62 b was performed using spectroscopic data obtained with the G141 grism (1.088 −1.68 μm).

TL;DR: In this paper, the atmospheric characterisation of three large, gaseous planets: WASP-127 b, wasP-79 b, and wasP62 b were analyzed using the Wide Field Camera 3 (WFC3) onboard the Hubble Space Telescope (HST) using the Iraclis pipeline and the TauREx3 retrieval code, both of which are publicly available.

TL;DR: In this article, the authors present an atmospheric characterization study of two medium sized planets bracketing the radius of Neptune: HD 106315 c (R$\rm{P}}$=4.23 R$\oplus}$) and HD 3167 c(R${P}$=2.17$\sigma$).

TL;DR: In this paper, a near-infrared transmission spectrum of the exo-Saturn WASP-117b was analyzed with two independent pipelines, and the authors reported the robust detection of a water spectral feature.