32 30 53 6 79 document 53 basu_chaplin_data.tar.gz application/x-gzip d7d23bd4fa0046f3db38d19dd481e20c MD5 27779562 2017-06-10 14:21:17 http://edata.bham.ac.uk/32/1/basu_chaplin_data.tar.gz 32 1 2 application/x-gzip application/x-gzip en public cc_by_4

basu_chaplin_data.tar.gz

54 6 80 document 54 basu_chaplin_answers.tar.gz application/x-gzip 56500f1a928e1e589d68d829bf5202c6 MD5 199227 2017-06-10 14:34:46 http://edata.bham.ac.uk/32/2/basu_chaplin_answers.tar.gz 32 2 1 application/x-gzip application/x-gzip en public cc_by_4

basu_chaplin_answers.tar.gz

archive 4 disk0/00/00/00/32 2017-06-13 14:10:19 2018-09-03 16:34:30 2018-05-24 15:01:51 dataset show 0 Basu Sarbani sarbani.basu@yale.edu Chaplin William J. w.j.chaplin@bham.ac.uk Department of Astronomy, Yale University pub Q1 QB QC 10col_ephy Stars, stellar oscillations, asteroseismology, sounds of the stars, asteroseismic analysis, asteroseismic inferences The archive basu_chaplin_data.tar.gz contains the synthetic data needed to solve the Exercise sets in the book: "Asteroseismic Data Analysis: Foundations and Techniques". The archive basu_chaplin_answers.tar.gz contains a PDF detailing the answers to the Exercise questions that are not open-ended. All data files are ASCII format. Here are some notes about the file formats, these can also be read in file README.txt: (1) Unless otherwise mentioned, the files with mode frequencies of modes have the format: l, n, frequency, Inl (2) Files with observed frequencies (or simulated observations) have the format l, n, frequency, uncertainty (3) Files in the archive freq_obs.tar have the formal l, frequency, uncertainty (4) Files Kernels_gs98_c2_rho.txt and Kernels_gs98_rho_c2.txt have the following information: Row 1: R, M Row 2: nr, (radius(i),i=1,nr) Row 3 onwards: l, n, frequency (kernel(i),i=1,nr) (5) The frequency files in the archives frequencies_ov[0-2].tar.gz have the following format l, n, frequency, Inl, np, ng (5) The rotational kernel files have the following format Row 1: R, M Row 2: nr, (radius(i),i=1, nr) Row 3 onwards: l, np, ng, frequency (kernel(i),i=1, nr) 2017 published University of Birmingham 10.5281/zenodo.807743 Dataset research-data@contacts.bham.ac.uk School of Physics and Astronomy BiSON - Birmingham Solar Oscillations Network NASA Kepler Mission na na na TRUE ds_ext http://bit.ly/Basu_and_Chaplin web http://www.birmingham.ac.uk/sasp pub https://press.princeton.edu/titles/11170.html