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Table · dataset · 2022

WASP-94A light curves

Listed in IVOA Registry (Virtual Observatory)

We present an optical transmission spectrum for WASP-94A b, the first atmospheric characterization of this highly-inflated hot Jupiter.

Description

The planet has a reported radius of 1.72^+0.06^_-0.05_R_Jup_, a mass of only 0.456^+0.032^_-0.036_M_Jup_, and an equilibrium temperature of 1508+/-75K. We observed the planet transit spectroscopically with the EFOSC2 instrument on the ESO New Technology Telescope (NTT) at La Silla, Chile: the first use of NTT/EFOSC2 for transmission spectroscopy.

We achieved an average transit-depth precision of 128ppm for bin widths of ~200{AA}. This high precision was achieved in part by linking Gaussian Process hyperparameters across all wavelength bins. The resulting transmission spectrum, spanning a wavelength range of 3800-7140{AA}, exhibits a sodium absorption with a significance of 4.9{sigma}, suggesting a relatively cloud-free atmosphere.

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The sodium signal may be broadened, with a best-fitting width of 78^+67^_-32_{AA} in contrast to the instrumental resolution of 27.2+/-0.2{AA}. We also detect a steep slope in the blue end of the transmission spectrum, indicating the presence of Rayleigh scattering in the atmosphere of WASP-94A b. Retrieval models show evidence for the observed slope to be super-Rayleigh and potential causes are discussed.

Finally, we find narrow absorption cores in the CaII H&K lines of WASP-94A, suggesting the star is enshrouded in gas escaping the hot Jupiter.

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Astronomical sciences 71%
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