Poster
M. Lundkvist, H. Kjeldsen, J. Christensen-Dalsgaard, T. L. Campante
Abstract
I have studied the two solar-like stars KIC-10273246 and KIC-11395018, also known as "Mulder" and "Boogie" respectively. I have developed an algorithm to compute the power spectrum of each of the two stars and I have done peak-bagging on these through the use of a fit to the power spectrum using the maximum likelihood approach. The found frequencies are compared to theoretically calculated frequencies and excellent agreement is expected.
Third Kepler Asteroseismology Workshop: 'Kepler Asteroseismology in Action'
Aarhus, Denmark
2010 June
