version=pmwiki-2.2.54 ordered=1 urlencoded=1
agent=Mozilla/5.0 (X11; Linux x86_64; rv:33.0) Gecko/20100101 Firefox/33.0
author=weiss
charset=UTF-8
csum=
ctime=1401982008
host=130.183.84.141
name=PmWiki.Proj34
rev=3
targets=
text='''Detection of signatures of binarity in oscillation spectra of non-eclipsing red giants'''%0a%0aEntry date: 07/01/2011%0a%0aStatus: Ongoing%0a%0aLead group: Birmingham%0a%0aCollaborating groups: Amsterdam, Saclay, Sydney%0a%0aContact person: Bill Chaplin%0a%0aCoordinating chair: Achim Weiss%0a%0aKepler data: Q0-Q5 time series of red giants.%0a%0aContent: %0a*Use population synthesis predictions to investigate for how many unresolved non-eclipsing binaries in the Kepler field we expect to be able to observe solar-like oscillations in both components.%0a*Use artificial data to tune data-analysis pipelines to see what signal we are able to pick-up in non-eclipsing binary giants with superposed oscillation signals%0a*Search for such binary non-eclipsing red giant stars in the Kepler FOV%0a*Investigate what we can learn from this binary population %0a%0aRemarks:%0a*This is a joint project with WG1 PE5.3%0a%0aMilestones:%0a*First paper with theoretical predictions [[http://adsabs.harvard.edu/abs/2014ApJ...784L...3M|published]]%0a%0aUpdate 17/11/14%0a*Search for binarity and double oscillation signal in lightcurve on-going.
time=1416219995
author:1416219995=weiss
diff:1416219995:1403768970:=27,30c27%0a%3c *First paper with theoretical predictions [[http://adsabs.harvard.edu/abs/2014ApJ...784L...3M|published]]%0a%3c %0a%3c Update 17/11/14%0a%3c *Search for binarity and double oscillation signal in lightcurve on-going.%0a\ No newline at end of file%0a---%0a> *First paper with theoretical predictions [[http://adsabs.harvard.edu/abs/2014ApJ...784L...3M|published]]%0a\ No newline at end of file%0a
host:1416219995=130.183.84.141
author:1403768970=admin
diff:1403768970:1401982008:=1,27d0%0a%3c '''Detection of signatures of binarity in oscillation spectra of non-eclipsing red giants'''%0a%3c %0a%3c Entry date: 07/01/2011%0a%3c %0a%3c Status: Ongoing%0a%3c %0a%3c Lead group: Birmingham%0a%3c %0a%3c Collaborating groups: Amsterdam, Saclay, Sydney%0a%3c %0a%3c Contact person: Bill Chaplin%0a%3c %0a%3c Coordinating chair: Achim Weiss%0a%3c %0a%3c Kepler data: Q0-Q5 time series of red giants.%0a%3c %0a%3c Content: %0a%3c *Use population synthesis predictions to investigate for how many unresolved non-eclipsing binaries in the Kepler field we expect to be able to observe solar-like oscillations in both components.%0a%3c *Use artificial data to tune data-analysis pipelines to see what signal we are able to pick-up in non-eclipsing binary giants with superposed oscillation signals%0a%3c *Search for such binary non-eclipsing red giant stars in the Kepler FOV%0a%3c *Investigate what we can learn from this binary population %0a%3c %0a%3c Remarks:%0a%3c *This is a joint project with WG1 PE5.3%0a%3c %0a%3c Milestones:%0a%3c *First paper with theoretical predictions [[http://adsabs.harvard.edu/abs/2014ApJ...784L...3M|published]]%0a\ No newline at end of file%0a
host:1403768970=130.183.84.141
author:1401982008=admin
diff:1401982008:1401982008:=
host:1401982008=130.183.84.141