Spectral and atmospheric characterization of 51 Eridani b using VLT/SPHERE
51 Eridani b is an exoplanet around a young (20 Myr) nearby (29.4 pc) F0-type star, recently discovered by direct imaging. Being only 0.5" away from its host star it is well suited for spectroscopic analysis using integral field spectrographs. We aim to refine the atmospheric properties of this...
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| Main Authors: | , |
|---|---|
| Format: | Article (Journal) Chapter/Article |
| Language: | English |
| Published: |
April 12, 2017
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| In: |
Arxiv
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| Online Access: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1704.02987
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| Author Notes: | M. Samland, P. Mollière, M. Bonnefoy, A.-L. Maire, F. Cantalloube, A.C. Cheetham, D. Mesa, R. Gratton, B.A. Biller, Z. Wahhaj, J. Bouwman, W. Brandner, D. Melnick, J. Carson, M. Janson, T. Henning, D. Homeier, C. Mordasini, M. Langlois, S.P. Quanz, R. van Boekel, A. Zurlo, J.E. Schlieder, H. Avenhaus, A. Boccaletti, M. Bonavita, G. Chauvin, R. Claudi, M. Cudel, S. Desidera, M. Feldt, R. Galicher, T.G. Kopytova, A.-M. Lagrange, H. Le Coroller, D. Mouillet, L. M. Mugnier, C. Perrot, E. Sissa, and A. Vigan |
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