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The Impact of Gaia and LSST on Binaries and Exoplanets

Published online by Cambridge University Press:  23 April 2012

L. Eyer
Affiliation:
Geneva Observatory, University of Geneva, Sauverny, Switzerland
P. Dubath
Affiliation:
ISDC, Geneva observatory, University of Geneva, Versoix, Switzerland
N. Mowlavi
Affiliation:
ISDC, Geneva observatory, University of Geneva, Versoix, Switzerland
P. North
Affiliation:
LASTRO, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, Versoix, Switzerland
A. Triaud
Affiliation:
Geneva Observatory, University of Geneva, Sauverny, Switzerland
F. Barblan
Affiliation:
Geneva Observatory, University of Geneva, Sauverny, Switzerland
C. Siopis
Affiliation:
IAA, Université Libre de Bruxelles, Bruxelles, Belgium
L. Guy
Affiliation:
ISDC, Geneva observatory, University of Geneva, Versoix, Switzerland
B. Tingley
Affiliation:
Instituto de Astrof-sica de Canarias, La Laguna, Spain
S. Zucker
Affiliation:
Department of Geophysics & Planetary Sciences, Tel Aviv University, Tel Aviv, Israel
D.W. Evans
Affiliation:
Institute of Astronomy, University of Cambridge, UK
L. Wyrzykowski
Affiliation:
Institute of Astronomy, University of Cambridge, UK Warsaw University Observatory, Warsaw, Poland
M. Süveges
Affiliation:
ISDC, Geneva observatory, University of Geneva, Versoix, Switzerland
Z. Ivezic
Affiliation:
Department of Astronomy, University of Washington, Seattle, USA
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Abstract

Two upcoming large scale surveys, the ESA Gaia and LSST projects, will bring a new era in astronomy. The number of binary systems that will be observed and detected by these projects is enormous, estimations range from millions for Gaia to several tens of millions for LSST. We review some tools that should be developed and also what can be gained from these missions on the subject of binaries and exoplanets from the astrometry, photometry, radial velocity and their alert systems.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2012

References

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