Asteroseismic Data Analysis: Foundations And Techniques

<strong>This site contains data needed to solve the Exercise sets in the book: "<em>Asteroseismic Data Analysis: Foundations and Techniques</em>".</strong> The archive Basu_and_Chaplin_Data.tar.gz contains the synthetic data.<br> The file archive answers.pdf contains a PDF detailing the answers to the Exercise questions that are not open-ended.<br> <br> All data files are ASCII format.<br> <br> Here are some notes about the file formats, these can also be read in file README.txt:<br> <br> (1) Unless otherwise mentioned, the files with mode frequencies of modes have the format:<br> l, n, frequency, Inl<br> <br> (2) Files with observed frequencies (or simulated observations) have the format<br> l, n, frequency, uncertainty<br> <br> (3) Files in the archive freq_obs.tar have the formal<br> l, frequency, uncertainty<br> <br> (4) Files Kernels_gs98_c2_rho.txt and Kernels_gs98_rho_c2.txt have the following information:<br> <br> Row 1: R, M<br> Row 2: nr, (radius(i),i=1,nr)<br> Row 3 onwards: l, n, frequency (kernel(i),i=1,nr)<br> <br> (5) The frequency files in the archives frequencies_ov[0-2].tar.gz have the following format<br> <br> l, n, frequency, Inl, np, ng<br> <br> (6) The rotational kernel files have the following format<br> <br> Row 1: R, M<br> Row 2: nr, (radius(i),i=1, nr)<br> Row 3 onwards: l, np, ng, frequency (kernel(i),i=1, nr)