A&A 564, A58 (2014) Astronomy DOI: 10.1051/0004-6361/201323041 & c ESO 2014 Astrophysics The Earth as an extrasolar transiting planet II. HARPS and UVES detection of water vapour, biogenic O2,andO3 L. Arnold1, D. Ehrenreich2, A. Vidal-Madjar3, X. Dumusque4, C. Nitschelm5,R.R.Querel6,7,P.Hedelt8, J. Berthier9, C. Lovis2, C. Moutou10,11,R.Ferlet3, and D. Crooker12 1 Aix Marseille Université, CNRS, OHP (Observatoire de Haute Provence), Institut Pythéas (UMS 3470), 04870 Saint-Michel-l’Observatoire, France e-mail:
[email protected] 2 Observatoire de Genève, Université de Genève, 51 ch. des Maillettes, 1290 Sauverny, Switzerland 3 Institut d’Astrophysique de Paris, UMR7095 CNRS, Université Pierre & Marie Curie, 98bis Boulevard Arago, 75014 Paris, France 4 Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, 02138 Cambridge, USA 5 Unidad de Astronomía, Facultad de Ciencias Básicas, Universidad de Antofagasta, 601 Avenida Angamos, Antofagasta, Chile 6 University of Chile, Department of Electrical Engineering, 2007 Tupper Avenue, Santiago, Chile 7 National Institute of Water and Atmospheric Research (NIWA), 1010 Auchland, Lauder, New Zealand 8 Deutsches Zentrum für Luft und Raumfahrt e.V. (DLR), Oberpfaffenhofen, 82234 Wessling, Germany 9 Institut de Mécanique Céleste et de Calcul des Éphémérides, Observatoire de Paris, Avenue Denfert-Rochereau, 75014 Paris, France 10 Aix Marseille Université, CNRS, LAM (Laboratoire d’Astrophysique de Marseille) UMR 7326, 13388 Marseille, France 11 CFHT Corporation, 65-1238 Mamalahoa Hwy Kamuela, Hawaii 96743, USA 12 Astronomy Department, Universidad de Chile, Casilla 36-D Santiago, Chile Received 7 November 2013 / Accepted 3 February 2014 ABSTRACT Context. The atmospheric composition of transiting exoplanets can be characterized during transit by spectroscopy.