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COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses

Published online by Cambridge University Press:  15 June 2005

F. Courbin
Affiliation:
Laboratoire d'Astrophysique de l'Ecole Polytechnique Fédérale de Lausanne, Observatoire, 1290 Chavannes-des-bois, Switzerland.
A. Eigenbrod
Affiliation:
Laboratoire d'Astrophysique de l'Ecole Polytechnique Fédérale de Lausanne, Observatoire, 1290 Chavannes-des-bois, Switzerland.
C. Vuissoz
Affiliation:
Laboratoire d'Astrophysique de l'Ecole Polytechnique Fédérale de Lausanne, Observatoire, 1290 Chavannes-des-bois, Switzerland.
G. Meylan
Affiliation:
Laboratoire d'Astrophysique de l'Ecole Polytechnique Fédérale de Lausanne, Observatoire, 1290 Chavannes-des-bois, Switzerland.
P. Magain
Affiliation:
Institut d'Astrophysique et de Géophysique, Université de Liège, Allée du 6 août 17, Sart Tilman Bat B5C, Liège, Belgium.
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Abstract

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We describe a new project aiming at measuring time delays for most known lensed quasars, from optical light curves obtained with five (almost) dedicated 1-2 m telescopes in the Northern and Southern hemispheres. The goal is to evaluate the Hubble constant H$_0$ with a precision below 2%. We present here numerical simulations in order to define the optimal temporal sampling in our observations as a function of typical quasar variations, object visibility, and for a given accuracy on the individual photometric points. It is also emphasized that the ongoing effort to obtain deep imaging using both space and ground based facilities must be continued, as illustrated by the comparison of HST and VLT near-IR images of the “cloverleaf”: H 1413+117.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Copyright
© 2004 International Astronomical Union