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Astron. Astrophys. 361, 877-887 (2000)

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Acknowledgements

The restoration of the images to sub-arcsecond resolutions and the corresponding photometry was possible only through the use of the MCS deconvolution algorithm. We are indebted to Dr. Pierre Magain (Institut d'Astrophysique et de Géophysique de Liège, Belgium) and Dr. Frédéric Courbin (Pontificia Universidad Católica, Chile) for making the algorithm available to us and for advice. The authors express their thanks to Dr. Georges Meynet for providing the models of the Geneva group. PR and GR are greatly indebted to the Fonds National de la Recherche Scientifique (Belgium) for multiple supports. They are also supported in part by contract P4/05 "Pôle d'Attraction Interuniversitaire" (SSTC-Belgium) and by the PRODEX XMM-OM Project.

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© European Southern Observatory (ESO) 2000

Online publication: January 29, 2001
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