ACCESS: An optical transmission spectrum of the high-gravity hot jupiter HAT-P-23b

Ian C. Weaver, Mercedes López-Morales, Munazza K. Alam, Néstor Espinoza, Benjamin V. Rackham, Jayesh M. Goyal, Ryan J. MacDonald, Nikole K. Lewis, Dániel Apai, Alex Bixel, Andrés Jordán, James Kirk, Chima McGruder, David J. Osip

Producción científica: Contribución a una revistaArtículorevisión exhaustiva

9 Citas (Scopus)


We present a new ground-based visible transmission spectrum of the high-gravity, hot Jupiter HAT-P-23b, obtained as part of the ACCESS project. We derive the spectrum from five transits observed between 2016 and 2018, with combined wavelength coverage between 5200 Å and 9269 Å in 200 Å bins, and with a median precision of 247 ppm per bin. HAT-P-23b’s relatively high surface gravity (g ≈ 30 m s−2), combined with updated stellar and planetary parameters from Gaia DR2, gives a five-scale-height signal of 384 ppm for a hydrogen-dominated atmosphere. Bayesian models favor a clear atmosphere for the planet with the tentative presence of TiO, after simultaneously modeling stellar contamination, using spots parameter constraints from photometry. If confirmed, HAT-P-23b would be the first example of a high-gravity gas giant with a clear atmosphere observed in transmission at optical/near-IR wavelengths; therefore, we recommend expanding observations to the UV and IR to confirm our results and further characterize this planet. This result demonstrates how combining transmission spectroscopy of exoplanet atmospheres with long-term photometric monitoring of the host stars can help disentangle the exoplanet and stellar activity signals.

Idioma originalInglés
Número de artículo278
PublicaciónAstronomical Journal
EstadoPublicada - jun. 2021
Publicado de forma externa


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