Gaia PS

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  • To refine the GAIA case for extrasolar planets (differentiate among different planetary formation models; planetary frequency with age; systems which can support life)
  • To evaluate the impact of photometric and astrometric noise intrinsic to the sources
  • To provide corresponding inputs to accuracy requirements and payload design
  • To provide inputs to the simulation task
  • To define optimal methods for the detection of candidate systems
  • To evaluate the combination of GAIA photometry, spectroscopy, and preliminary parallax data to optimize the candidate list
  • To assess the need for detectability requirements at the level of core processing
  • To establish methods for orbital fiting (including strategies for finding initial values of orbital parameters)
  • To perform extensive simulations of detection and orbit determination (including double-blind tests)
  • To develop a reduction model for the parallel processing (algorithms, inputs, outputs)
  • To establish needs and capabilities for ground-based follow-up observations

http://wwwhip.obspm.fr/gaia/ps $RCSfile: tasks.html,v $, $Revision: 1.1 $