OverSampling Mode

1
OverSampling Mode

• Criteria for list of target management

2
Initial List of targets

• 1000 possibilities for oversampling
• Initial list of targets
• For the AP-side TBD by the APWG
• For the ExoSide
• Stars known to host a planet from ground based
  observations
• Stars selected as references over the HR diagram
• ? calibration of the stellar variability
• (for improving detection in the LCs).
• Priority is left progressively to targets of the
  OSM

3
Few principles to make criteria

• For a given method candidates are sorted
  following confidence level in the detection
• Periodic candidates globally have higher
  confidence level than single events
• Periodic events detected by 2 methods are more
  secure detections than by a single one
• Eclipsing Binaries do not have the same interest
  as Planetary candidates (second order interest
  ).

4
Proposed priorities

• - P1 candidates common to BLS and MIDEPF
• (periodic events detected by the 2 methods)
• - P2 candidates obtained with BLS only
• (periodic event detected by the standard
  method)
• - P3 candidates obtained with only MIDEPF
• (low periodicity weak transit number)
• - P4 candidates obtained with only MID
• (single transit feature)
• - P5 confirmed Eclipsing Binaries

5
Role of the SOS

• The role of the Scientific Oversampling Staff
  (SOS) is
• To check the scientific consistency of the list
  of targets to be oversampled
• To change some of the priorities issued from the
  software
• To attribute the highest priority P0 to some
  peculiar events