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The {\\beta} Pictoris system offers the rare opportunity to study the physical and atmospheric properties of an exoplanet placed on a wide orbit and to establish its formation scenario. We obtained J (1.265 {\\mu}m), H (1.66 {\\mu}m), and M' (4.78 {\\mu}m) band angular differential imaging of the system between 2011 and 2012. We detect the planetary companion in our four-epoch observations. We estimate J = 14.0 +- 0.3, H = 13.5 +- 0.2, and M' = 11.0 +- 0.3 mag. 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Boccaletti, A.-M. Lagrange, C. Mordasini, D. Apai, D. Homeier, D. Rouan, F. Allard, G. Chauvin, H. Beust, J. H. V. Girard, M. Bonnefoy, S. Lacour","submitted_at":"2013-02-05T19:31:53Z","abstract_excerpt":"A gas giant planet has previously been directly seen orbiting at 8-10 AU within the debris disk of the ~12 Myr old star {\\beta} Pictoris. The {\\beta} Pictoris system offers the rare opportunity to study the physical and atmospheric properties of an exoplanet placed on a wide orbit and to establish its formation scenario. We obtained J (1.265 {\\mu}m), H (1.66 {\\mu}m), and M' (4.78 {\\mu}m) band angular differential imaging of the system between 2011 and 2012. We detect the planetary companion in our four-epoch observations. We estimate J = 14.0 +- 0.3, H = 13.5 +- 0.2, and M' = 11.0 +- 0.3 mag. 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