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COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses

E. EulaersInstitut d’Astrophysique et de Géophysique, Université de Liège, 17 Allée du 6 Août, Sart Tilman (Bat. B5C), Liège 1, BelgiumM. TewesLaboratoire d’Astrophysique, École Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, 1290 Versoix, SwitzerlandPierre MagainInstitut d’Astrophysique et de Géophysique, Université de Liège, 17 Allée du 6 Août, Sart Tilman (Bat. B5C), Liège 1, BelgiumF. CourbinLaboratoire d’Astrophysique, École Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, 1290 Versoix, SwitzerlandI. M. AsfandiyarovUlugh Beg Astronomical Institute, Uzbek Academy of Sciences, Astronomicheskaya 33, 100052 Tashkent, UzbekistanSh. A. EhgamberdievUlugh Beg Astronomical Institute, Uzbek Academy of Sciences, Astronomicheskaya 33, 100052 Tashkent, UzbekistanSushil KumarIndian Institute of Astrophysics, II Block, Koramangala, 560 034 Bangalore, IndiaC. S. StalinIndian Institute of Astrophysics, II Block, Koramangala, 560 034 Bangalore, IndiaT. P. PrabhuIndian Institute of Astrophysics, II Block, Koramangala, 560 034 Bangalore, IndiaG. MeylanLaboratoire d’Astrophysique, École Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, 1290 Versoix, SwitzerlandH. Van WinckelInstituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200B, 3001 Heverlee, Belgium
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Aims. Within the framework of the COSMOGRAIL collaboration we present 7- and 8.5-year-long light curves and time-delay estimates for two gravitationally lensed quasars: SDSS J1206+4332 and HS 2209+1914.

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