Reference : Prospects for Near-infrared Characterisation of Hot Jupiters with the VLTI Spectro-image...
Scientific congresses and symposiums : Paper published in a book
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/22520
Prospects for Near-infrared Characterisation of Hot Jupiters with the VLTI Spectro-imager (VSI)
English
Renard, Stéphanie [Université Joseph Fourier - Grenoble 1 - UJF > Laboratoire d'Astrophysique de Grenoble > > >]
Absil, Olivier mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS) >]
Berger, Jean-Philippe [> > > >]
Bonfils, Xavier [> > > >]
Forveille, Thierry [> > > >]
Malbet, Fabien [> > > >]
2009
Science with the VLT in the ELT Era
Moorwood, A.
Springer
Astrophysics and Space Science Proceedings
349-351
No
No
International
Dordrecht
Netherlands
Science with the VLT in the ELT Era
du 8 au 12 octobre 2007
ESO
Garching
Germany
[en] Since the discovery of the first exoplanet around 51 Pegasi, the study of planetary systems receives an increasing attention, with the development and test of more and more detection techniques. Among the direct detection techniques, interferometry is one of the most promising for the near future. It already provides the required angular resolution, but the dynamic range needs to be improved. The detection and characterisation of extrasolar planets is one of the main science cases of the 2nd generation VLTI Spectro-Imager instrument (VSI). The goal of this work is to study the feasibility of obtaining near-infrared spectra of bright extrasolar giant planets (EGP) with VSI.
Researchers
http://hdl.handle.net/2268/22520
10.1007/978-1-4020-9190-2_58
http://adsabs.harvard.edu/abs/2009svlt.conf..349R

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