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The ESPRI project: narrow-angle astrometry with VLTI-PRIMA

Published online by Cambridge University Press:  01 October 2007

R. Launhardt*
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany
T. Henning
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany
D. Queloz
Affiliation:
Observatoire Astronomique de l'Universitè de Genève, 1290 Sauverny, Switzerland
A. Quirrenbach
Affiliation:
Landessternwarte Königstuhl, 69117 Heidelberg, Germany
F. Delplancke
Affiliation:
European Southern Observatory (ESO), Karl-Schwazschild-Str. 2, 85748 Garching
N. M. Elias II
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany Landessternwarte Königstuhl, 69117 Heidelberg, Germany
F. Pepe
Affiliation:
Observatoire Astronomique de l'Universitè de Genève, 1290 Sauverny, Switzerland
S. Reffert
Affiliation:
Landessternwarte Königstuhl, 69117 Heidelberg, Germany
D. Ségransan
Affiliation:
Observatoire Astronomique de l'Universitè de Genève, 1290 Sauverny, Switzerland
J. Setiawan
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany
R. Tubbs
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany
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Abstract

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We describe the ongoing hardware and software developments that shall enable the ESO VLTI to perform narrow-angle differential delay astrometry in K-band with an accuracy of up to 10 μarcsec. The ultimate goal of these efforts is to perform an astrometric search for extrasolar planets around nearby stars.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2008

References

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