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^<fc #800080>Objectives Summary</fc>||||||
^#                ^Brief Description   ^Period ^Dependency ^Milestone ^Deliverable|
|1 | Self-consistent analysis of photometric lightcurves | M01-M36 |- |-|-|
|1.1 | Impact of gaps in the harmonic analysis  |M01-M12|-|-|-|
|1.2 | Adaptation of OleMIARMA software to PLATO2.0 pipeline| M12-M36 |-|-|-|
|1.3 | Characterization of convection through frequency content | M12-M24 |-|-|-|
|2  | Extend the analysis of modal identification to IR   | M12-M24 |-|-|-|
|3  | Development of quasi-simultenous VIS-IR observing mode for mode identification with OSN facilities |M12-24|-|-|-|
|4  | Participation of OSN in FU activities up to PDR | M12-M24|-|-|-|

=== Objective #1 Analysis of photometric lightcurves ===
- Problem of gaps in the sampling. No measures (zero) is even worst. Linear interpolation
is equivalent to zeros. 
- Even without gaps there is a so-called red-noise. Characterization of such a noise.
- relate with WPs of PDC
- Using legacy data from Corot and Kepler we propose a proper analysis for PLATO2.0 data. 


=== Objective #2 Extend the analysis of modal identification to IR  ===
-This would be the topic for PhD
-

=== Objective #3 More stuff to be done ===
- Software development (Nacho) 

=== Objective #5 FU ===
- Susana. Nacho : registrarse en la web. Contacto con el responsable.
-

=== Support stuff ===
- include relation between PLATO and CARMENES. RV (Thoundsen code, Cristina); characterisation of A-F stars with planets
-