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text=Entry date: 15/12/2011%0a%0aStatus: Ongoing%0a%0aLead group: Birmingham%0a%0aCollaborating groups: Amsterdam%0a%0aContact person: Bill Chaplin%0a%0aCoordinating subchair: Yvonne Elsworth%0a%0aKepler data: all Q time series of Kepler targets classified as M-dwarfs%0a%0aContent: %0a*Preliminary studies on the accuracy of the KIC parameters for M dwarfs indicate that as many as 95%25 of the bright Kepler M dwarfs may actually be red giant stars%0a*We will reprocess all Kepler targets which the KIC classifies as M dwarfs, to check their Fourier spectrum, and flag those stars with the seismic properties of a giant. %0a%0aPrerequisites: %0a*None%0a%0aRemarks:%0a*This project is carried out in collaboration with WG1.%0a%0aJournal:%0a*MNRAS
time=1399319867
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diff:1399319867:1399319867:=1,26d0%0a%3c Entry date: 15/12/2011%0a%3c %0a%3c Status: Ongoing%0a%3c %0a%3c Lead group: Birmingham%0a%3c %0a%3c Collaborating groups: Amsterdam%0a%3c %0a%3c Contact person: Bill Chaplin%0a%3c %0a%3c Coordinating subchair: Yvonne Elsworth%0a%3c %0a%3c Kepler data: all Q time series of Kepler targets classified as M-dwarfs%0a%3c %0a%3c Content: %0a%3c *Preliminary studies on the accuracy of the KIC parameters for M dwarfs indicate that as many as 95%25 of the bright Kepler M dwarfs may actually be red giant stars%0a%3c *We will reprocess all Kepler targets which the KIC classifies as M dwarfs, to check their Fourier spectrum, and flag those stars with the seismic properties of a giant. %0a%3c %0a%3c Prerequisites: %0a%3c *None%0a%3c %0a%3c Remarks:%0a%3c *This project is carried out in collaboration with WG1.%0a%3c %0a%3c Journal:%0a%3c *MNRAS%0a\ No newline at end of file%0a
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