output
20072024
most citedThe Transit Light Curve Project. IX. Evidence for a Smaller Radius of the Exoplanet XO-3b

327 citations

13 papers

astro-ph.EP2024★ 60 cited

The long-term steady motion of Saturn's Hexagon and the stability of its enclosed jet-stream under seasonal changes

A. Sánchez-Lavega, T. del Río-Gaztelurrutia, R. Hueso +15

We investigate the long-term motion of Saturn's North-Pole Hexagon and the structure of its associated eastward jet, using Cassini ISS and ground-based images from 2008 to 2014. We…

astro-ph.EP2024★ 27 cited

An Enduring Rapidly Moving Storm as a Guide to Saturn's Equatorial Jet's Complex Structure

A. Sánchez-Lavega, E. García-Melendo, S. Perez-Hoyos +14

Saturn has an intense and broad eastward equatorial jet with a complex three-dimensional structure mixed with time variability. The equatorial region experiences strong seasonal in…

astro-ph.EP2019★ 22 cited

Observations and numerical modelling of a convective disturbance in a large-scale cyclone in Jupiter's South Temperate Belt

P. Iñurrigarro, R. Hueso, J. Legarreta +8

Moist convective storms in Jupiter develop frequently and can trigger atmospheric activity of different scales, from localized storms to planetary-scale disturbances including conv…

astro-ph.EP2019★ 20 cited

Saturn atmospheric dynamics one year after Cassini: Long-lived features and time variations in the drift of the Hexagon

R. Hueso, A. Sánchez-Lavega, J. F. Rojas +15

We examine Saturn's atmosphere with observations from ground-based telescopes and Hubble Space Telescope (HST). We present a detailed analysis of observations acquired during 2018.…

astro-ph.EP2017★ 24 cited

Neptune long-lived atmospheric features in 2013-2015 from small (28-cm) to large (10-m) telescopes

R. Hueso, I. de Pater, A. Simon +32

Since 2013, observations of Neptune with small telescopes have resulted in several detections of long-lived bright atmospheric features that have also been observed by large telesc…

astro-ph.EP2017★ 47 cited

Discovery of XO-6b: a hot Jupiter transiting a fast rotating F5 star on an oblique orbit

N. Crouzet, P. R. McCullough, D. Long +20

Only a few hot Jupiters are known to orbit around fast rotating stars. These exoplanets are harder to detect and characterize and may be less common than around slow rotators. Here…