Corrigendum to "The upper atmosphere of the exoplanet HD209458b revealed by the sodium D lines: Temperature-pressure profile, ionization layer and thermosphere" [2011, A&A, 527, A110]
arXiv:1110.5750 · doi:10.1051/0004-6361/201015698e
Abstract
An error was detected in the code used for the analysis of the HD209458b sodium profile (Vidal-Madjar et al. 2011). Here we present an updated T-P profile and briefly discuss the consequences.
Published in Astronomy & Astrophysics, 533, C4
References in corpus (1)
Cited by in corpus (16)
- The escape of heavy atoms from the ionosphere of HD209458b. I. A photochemical-dynamical model of the thermosphere
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- Simulating the escaping atmospheres of hot gas planets in the solar neighborhood
- Hot Exoplanet Atmospheres Resolved with Transit Spectroscopy (HEARTS) - II. A broadened sodium feature on the ultra-hot giant WASP-76b
- Magnesium in the atmosphere of the planet HD209458b: Observations of the thermosphere-exosphere transition region
- Hot Exoplanet Atmospheres Resolved with Transit Spectroscopy (HEARTS) I. Detection of hot neutral sodium at high altitudes on WASP-49b
- GTC OSIRIS transiting exoplanet atmospheric survey: detection of sodium in XO-2b from differential long-slit spectroscopy
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- An HST/STIS Optical Transmission Spectrum of Warm Neptune GJ 436b
- On the sensitivity of extrasolar mass-loss rate ranges: HD 209458b a case study
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