The upper atmosphere of the exoplanet HD209458b revealed by the sodium D lines: temperature-pressure profile, ionization layer and thermosphere (Corrigendum)

A. Vidal-Madjar; C. M Huitson; A. Lecavelier des Etangs; D. K. Sing; R. Ferlet; J.-M. Désert; G. Hébrard; I. Boisse; D. Ehrenreich; C. Moutou

doi:doi:10.1051/0004-6361/201015698e

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This article is an erratum for: [this article]

Issue		A&A Volume 533, September 2011


Article Number		C4
Number of page(s)		2
Section		Planets and planetary systems
DOI		http://dx.doi.org/10.1051/0004-6361/201015698e
Published online		16 September 2011

A&A 533, C4 (2011)

The upper atmosphere of the exoplanet HD209458b revealed by the sodium D lines: temperature-pressure profile, ionization layer and thermosphere (Corrigendum)

A. Vidal-Madjar¹, C. M Huitson², A. Lecavelier des Etangs¹, D. K. Sing², R. Ferlet¹, J.-M. Désert³, G. Hébrard¹, I. Boisse¹, D. Ehrenreich⁴ and C. Moutou⁵

¹ CNRS, UPMC, Institut d’astrophysique de Paris, UMR 7095, 98bis boulevard Arago, 75014 Paris, France
e-mail: alfred@iap.fr
² Astrophysics Group, School of Physics, University of Exeter, Stocker Road, Exeter EX4 4QL, UK
³ Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA
⁴ Laboratoire d’Astrophysique de Grenoble, Université Joseph Fourier, CNRS (UMR 5571), BP 53, 38041 Grenoble Cedex 9, France
⁵ Laboratoire d’Astrophysique de Marseille,Technopôle Marseille Étoile, 38 rue Frédéric Joliot Curie, 13013 Marseille, France

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.

Key words: methods: observational / techniques: spectroscopic / planets and satellites: atmospheres / methods: data analysis / Errata, addenda / stars: individual: HD209458

Erratum of: A&A 527, A110 (2011), DOI: 10.1051/0004-6361/201015698

© ESO, 2011

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