Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Earth and Planetary Astrophysics
Scientist
Laboratoire de Physique de l'Université de Bourgogne, Dijon, France
Laboratoire de Physique de l'Université de Bourgogne, CNRS UMR 5027, Boîte Postale 47870, F-21078 Dijon, France
Laboratoire Interdisciplinaire Carnot de Bourgogne, UMR 5209 CNRS-Université de Bourgogne, 9. Av. A. Savary, BP 47870, F-21078 Dijon Cedex, France
l'Université de Bourgogne, France
ICB, University of Dijon, France
Institut Carnot de Bourgogne, Université de Bourgogne, France
Laboratoire de Physique de l'Universitéde Bourgogne, Dijon, France
Laboratoire Interdisciplinaire Carnot de Bourgogne, UMR 5209 CNRS-Université de Bourgogne, 9 Av. Savary, BP 47870, F21078 Dijon Cedex, France
Institut Carnot de Bourgogne, UMR 5209 CNRS-Université de Bourgogne, 9. Av. A. Savary, BP 47870, F-21078 Dijon Cedex, France
Groupe de Spectrométrie Moléculaire et Atmosphérique -- GSMA
Laboratoire interdisciplinaire Carnot de Bourgogne, UMR 5209 CNRS--Université de Bourgogne, 9, Avenue Alain Savary, BP 47870, F-21078 Dijon Cedex, France
Institut Carnot de Bourgogne, UMR CNRS 5209, 9 avenue Alain Savary, BP 47870, 21078 Dijon Cedex, France
Institut Carnot de Bourgogne, UMR 5209 CNRS-Université de Bourgogne, 9 Av. A. Savary, BP 47870, F-21078 Dijon Cedex, France
ICB, Univ. Dijon, FRANCE
Institut Carnot de Bourgogne, UMR 5209 CNRS-Université de Bourgogne, 9 Av.A. Savary, BP 47870, F-21078 Dijon Cedex, France
Institut Carnot de Bourgogne UMR 5209 CNRS, Université de Bourgogne, Dijon, France
A new analysis of the ESO Very Large Telescope (VLT) observations of Titan's at 2 µm.
A new analysis of the ESO Very Large Telescope (VLT) observations of Titan's at 2 μm.
Application of new methane linelists to Cassini and Earth-based data of Titan.
Applications of a new set of methane line parameters to the modeling of Titan's spectrum in the 1.58 μm window
Breakdown of the Reduction of the Rovibrational Hamiltonian : the Case of S^{18}O_2F_2
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