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text=Entry date: 13/12/2011%0a%0aStatus: Ongoing%0a%0aLead group: Meudon%0a%0aCollaborating groups: Amsterdam, Birmingham, Leuven, Saclay, Sydney%0a%0aContact person: Benoit Mosser%0a%0aCoordinating chair: Yvonne Elsworth%0a%0aKepler data: All available quarters.%0a%0aContent: %0a*Measure the large separation at low frequency (lower than the red-clump value, down to 0.2, 0.3 muHz)%0a*Measure the mode visibility (as in Mosser et al.  2011)%0a*Investigate how the mode visibility varies with frequency when Dnu decreases%0a*If possible, measure the period spacing of mixed modes%0a*Disentangle RGB and AGB stars.%0a*A link will be established between the period-luminosity relations from ground-based measurement and solar-like oscillations seen by Kepler.%0a%0aRemarks:%0a*Different methods/pipelines will be used and compared.%0a*Because of their expertise with OGLE red giant stars, I. Soszynski and W. Dziembowski are involved in the project. %0a%0aPrerequisites:%0a*None%0a%0aMilestones:%0a*Results to be provided before March, 1, 2013: Dnu, numax, complete mode identification, mode heights, amplitudes, background, and visibilities V²(l)%0a*First draft of the paper: March 2013%0a*16/05/'13: first draft being discussed by co-authors.%0a%0aJournal:%0a*A&A%0a%0a*Files: [[Attach:P56.png|First Kepler Results]]
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diff:1399319557:1399319543:=38c38%0a%3c *Files: [[Attach:P56.png|First Kepler Results]]%0a\ No newline at end of file%0a---%0a> *Files: [[Attach:P56.png]|First Kepler Results]]%0a\ No newline at end of file%0a
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diff:1399319543:1399319494:=38c38%0a%3c *Files: [[Attach:P56.png]|First Kepler Results]]%0a\ No newline at end of file%0a---%0a> *Files: [[Attach:P56.png]|First Kepler Results]%0a\ No newline at end of file%0a
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diff:1399319494:1399319494:=1,38d0%0a%3c Entry date: 13/12/2011%0a%3c %0a%3c Status: Ongoing%0a%3c %0a%3c Lead group: Meudon%0a%3c %0a%3c Collaborating groups: Amsterdam, Birmingham, Leuven, Saclay, Sydney%0a%3c %0a%3c Contact person: Benoit Mosser%0a%3c %0a%3c Coordinating chair: Yvonne Elsworth%0a%3c %0a%3c Kepler data: All available quarters.%0a%3c %0a%3c Content: %0a%3c *Measure the large separation at low frequency (lower than the red-clump value, down to 0.2, 0.3 muHz)%0a%3c *Measure the mode visibility (as in Mosser et al.  2011)%0a%3c *Investigate how the mode visibility varies with frequency when Dnu decreases%0a%3c *If possible, measure the period spacing of mixed modes%0a%3c *Disentangle RGB and AGB stars.%0a%3c *A link will be established between the period-luminosity relations from ground-based measurement and solar-like oscillations seen by Kepler.%0a%3c %0a%3c Remarks:%0a%3c *Different methods/pipelines will be used and compared.%0a%3c *Because of their expertise with OGLE red giant stars, I. Soszynski and W. Dziembowski are involved in the project. %0a%3c %0a%3c Prerequisites:%0a%3c *None%0a%3c %0a%3c Milestones:%0a%3c *Results to be provided before March, 1, 2013: Dnu, numax, complete mode identification, mode heights, amplitudes, background, and visibilities V²(l)%0a%3c *First draft of the paper: March 2013%0a%3c *16/05/'13: first draft being discussed by co-authors.%0a%3c %0a%3c Journal:%0a%3c *A&A%0a%3c %0a%3c *Files: [[Attach:P56.png]|First Kepler Results]%0a\ No newline at end of file%0a
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