The near-infrared spectral energy distribution of β Pictoris b

@article{Bonnefoy2013TheNS,
  title={The near-infrared spectral energy distribution of $\beta$ Pictoris b},
  author={Micka{\"e}l Bonnefoy and Anthony Boccaletti and Anne-Marie Lagrange and France Allard and Christoph Mordasini and Herv'e Beust and Ga{\"e}l Chauvin and Julien H. Girard and Derek Homeier and D{\'a}niel Apai and Sylvestre Lacour and Daniel Rouan},
  journal={Astronomy and Astrophysics},
  year={2013},
  volume={555}
}
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… 
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