iMAC data set

================================================================================<br> Title: Comparison between core-collapse supernova nucleosynthesis and meteoric <br> stardust grains: investigating magnesium, aluminium, and chromium <br> Authors: den Hartogh J., Peto M.K., Lawson T., Sieverding A., Brinkman H., <br> Pignatari M., Lugaro M. <br> ================================================================================<br> Description of contents: the data files in this data deposit are either stellar profiles or stellar yields as used in the paper to create figures. All files are machine readable .txt files. Any text editor is able to open these files. A complete list of the files in this repository are provided here: iMAC_profiles/m15exp_LAW_D_subm.txt<br> iMAC_profiles/m15exp_LAW_R_subm.txt<br> iMAC_profiles/m15exp_RIT_D_subm.txt<br> iMAC_profiles/m15exp_RIT_R_subm.txt<br> iMAC_profiles/m15exp_SIE_D_subm.txt<br> iMAC_profiles/m15exp_SIE_R_subm.txt<br> iMAC_profiles/m20exp_LAW_D_subm.txt<br> iMAC_profiles/m20exp_LAW_R_subm.txt<br> iMAC_profiles/m20exp_RIT_D_subm.txt<br> iMAC_profiles/m20exp_RIT_R_subm.txt<br> iMAC_profiles/m20exp_SIE_D_subm.txt<br> iMAC_profiles/m20exp_SIE_R_subm.txt<br> iMAC_profiles/m25exp_LAW_D_subm.txt<br> iMAC_profiles/m25exp_LAW_R_subm.txt<br> iMAC_profiles/m25exp_RIT_D_subm.txt<br> iMAC_profiles/m25exp_RIT_R_subm.txt<br> iMAC_profiles/m25exp_SIE_D_subm.txt<br> iMAC_profiles/m25exp_SIE_R_subm.txt iMAC_yields/m15_yields_D.txt<br> iMAC_yields/m20_yields_D.txt<br> iMAC_yields/m25_yields_D.txt For the profiles the *R_subm.txt files have the following columns:<br> mass,he4,c12,o16,ne20,si28,ni56,fe56,al26,al27,mg24,mg25,mg26,cr50,cr52,cr53,cr54<br> All isotopes are radioactive or non-decayed. For the profiles the *D_subm.txt files have the following columns:<br> mass,al27,mg24,mg25,mg26,cr50,cr52,cr53,cr54<br> All isotopes include all radioactive contributions and are thus fully decayed. The yield files have the following columns:<br> ref Mg24, Mg25, Mg26, Al26, Al27, Cr50, Cr52, Cr53, Cr54<br> All yields are fully decayed. The refs are equal to the labels in Figure 2. <br> <br> <br> <br> System requirements: - Additional comments: the Cr53 data for the middle row of Figure 3 is not included in these files. ================================================================================